Japanese X-Ray Satellite to Probe Universe's Largest Structures

A revolutionary satellite is preparing to take to the skies, viewing the hidden parts of cosmos in a new light to reveal stellar explosions and powerful jets streaming from supermassive black holes. First Full-Color Images From Webb Space Telescope XRISM (X-ray Imaging and Spectroscopy Mission), a joint mission between the Japan Aerospace Exploration Agency (JAXA) and NASA, is designed to…

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The Milky Way's close neighbor, Andromeda, features a dominant source of high-energy X-ray emission, but its identity was mysterious until now. As reported in a new study, NASA's NuSTAR (Nuclear Spectroscopic Telescope Array) mission has pinpointed an object responsible for this high-energy radiation.

The object, called Swift J0042.6+4112, is a possible pulsar, the dense remnant of a dead star that is highly magnetized and spinning, researchers say. This interpretation is based on its emission in high-energy X-rays, which NuSTAR is uniquely capable of measuring. The object’s spectrum is very similar to known pulsars in the Milky Way.

It is likely in a binary system, in which material from a stellar companion gets pulled onto the pulsar, spewing high-energy radiation as the material heats up.

"We didn't know what it was until we looked at it with NuSTAR," said Mihoko Yukita, lead author of a study about the object, based at Johns Hopkins University in Baltimore. The study is published in The Astrophysical Journal.

This candidate pulsar is shown as a blue dot in a NuSTAR X-ray image of Andromeda (also called M31), where the color blue is chosen to represent the highest-energy X-rays. It appears brighter in high-energy X-rays than anything else in the galaxy.

The study brings together many different observations of the object from various spacecraft. In 2013, NASA's Swift satellite reported it as a high-energy source, but its classification was unknown, as there are many objects emitting low energy X-rays in the region. The lower-energy X-ray emission from the object turns out to be a source first identified in the 1970s by NASA’s Einstein Observatory. Other spacecraft, such as NASA's Chandra X-ray Observatory and ESA's XMM-Newton had also detected it. However, it wasn't until the new study by NuSTAR, aided by supporting Swift satellite data, that researchers realized it was the same object as this likely pulsar that dominates the high energy X-ray light of Andromeda.

Traditionally, astronomers have thought that actively feeding black holes, which are more massive than pulsars, usually dominate the high-energy X-ray light in galaxies. As gas spirals closer and closer to the black hole in a structure called an accretion disk, this material gets heated to extremely high temperatures and gives off high-energy radiation. This pulsar, which has a lower mass than any of Andromeda's black holes, is brighter at high energies than the galaxy's entire black hole population.

Even the supermassive black hole in the center of Andromeda does not have significant high-energy X-ray emission associated with it. It is unexpected that a single pulsar would instead be dominating the galaxy in high-energy X-ray light.

"NuSTAR has made us realize the general importance of pulsar systems as X-ray-emitting components of galaxies, and the possibility that the high energy X-ray light of Andromeda is dominated by a single pulsar system only adds to this emerging picture," said Ann Hornschemeier, co-author of the study and based at NASA's Goddard Space Flight Center, Greenbelt, Maryland.

Andromeda is a spiral galaxy slightly larger than the Milky Way. It resides 2.5 million light-years from our own galaxy, which is considered very close, given the broader scale of the universe. Stargazers can see Andromeda without a telescope on dark, clear nights.

"Since we can't get outside our galaxy and study it in an unbiased way, Andromeda is the closest thing we have to looking in a mirror," Hornschemeier said.

NuSTAR is a Small Explorer mission led by Caltech and managed by JPL for NASA's Science Mission Directorate in Washington. NuSTAR was developed in partnership with the Danish Technical University and the Italian Space Agency (ASI). The spacecraft was built by Orbital Sciences Corp., Dulles, Virginia. NuSTAR's mission operations center is at UC Berkeley, and the official data archive is at NASA's High Energy Astrophysics Science Archive Research Center. ASI provides the mission's ground station and a mirror archive. JPL is managed by Caltech for NASA.

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ANDROMEDA’S BRIGHT X-RAY MYSTERY SOLVED BY NUSTAR The Milky Way’s closest neighbor [of comparable size], [the] Andromeda [galaxy], features a dominant source of high-energy X-ray emission, but its identity was mysterious until now. As reported in a new study, NASA’s NuSTAR (Nuclear Spectroscopic Telescope Array) mission has pinpointed an object responsible for this high-energy radiation. The object, called Swift J0042.6+4112, is a possible pulsar, the dense remnant of a dead star that is highly magnetized and spinning, researchers say. This interpretation is based on its emission in high-energy X-rays, which NuSTAR is uniquely capable of measuring. The object’s spectrum is very similar to known pulsars in the Milky Way. It is likely in a binary system, in which material from a stellar companion gets pulled onto the pulsar, spewing high-energy radiation as the material heats up. “We didn’t know what it was until we looked at it with NuSTAR,” said Mihoko Yukita, lead author of a study about the object, based at Johns Hopkins University in Baltimore. The study is published in the Astrophysical Journal. This candidate pulsar is shown as a blue dot in a NuSTAR X-ray image of Andromeda (also called M31), where the color blue is chosen to represent the highest-energy X-rays. It appears brighter in high-energy X-rays than anything else in the galaxy. The study brings together many different observations of the object from various spacecraft. In 2013, NASA’s Swift satellite reported it as a high-energy source, but its classification was unknown, as there are many objects emitting low energy X-rays in the region. The lower-energy X-ray emission from the object turns out to be a source first identified in the 1970s by NASA’s Einstein Observatory. Other spacecraft, such as NASA’s Chandra X-ray Observatory and ESA’s XMM-Newton had also detected it. However, it wasn’t until the new study by NuSTAR, aided by supporting Swift satellite data, that researchers realized it was the same object as this likely pulsar that dominates the high energy X-ray light of Andromeda. Traditionally, astronomers have thought that actively feeding black holes, which are more massive than pulsars, usually dominate the high-energy X-ray light in galaxies. As gas spirals closer and closer to the black hole in a structure called an accretion disk, this material gets heated to extremely high temperatures and gives off high-energy radiation. This pulsar, which has a lower mass than any of Andromeda’s black holes, is brighter at high energies than the galaxy’s entire black hole population. Even the supermassive black hole in the center of Andromeda does not have significant high-energy X-ray emission associated with it. It is unexpected that a single pulsar would instead be dominating the galaxy in high-energy X-ray light. “NuSTAR has made us realize the general importance of pulsar systems as X-ray-emitting components of galaxies, and the possibility that the high energy X-ray light of Andromeda is dominated by a single pulsar system only adds to this emerging picture,” said Ann Hornschemeier, co-author of the study and based at NASA’s Goddard Space Flight Center, Greenbelt, Maryland. Andromeda is a spiral galaxy slightly larger than the Milky Way. It resides 2.5 million light-years from our own galaxy, which is considered very close, given the broader scale of the universe. Stargazers can see Andromeda without a telescope on dark, clear nights. “Since we can’t get outside our galaxy and study it in an unbiased way, Andromeda is the closest thing we have to looking in a mirror,” Hornschemeier said. IMAGE....NASA's Nuclear Spectroscope Telescope Array, or NuSTAR, has identified a candidate pulsar in Andromeda -- the nearest large galaxy to the Milky Way. This likely pulsar is brighter at high energies than the Andromeda galaxy's entire black hole population. The inset image shows the pulsar candidate in blue, as seen in X-ray light by NuSTAR. The background image of Andromeda was taken by NASA's Galaxy Evolution Explorer in ultraviolet light. Andromeda is a spiral galaxy like our Milky Way but larger in size. It lies 2.5 million light-years away in the Andromeda constellation.

Andromeda's Bright X-Ray Mystery Solved by NuSTAR

The Milky Way's close neighbor, Andromeda, features a dominant source of high-energy X-ray emission, but its identity was mysterious until now. As reported in a new study, NASA's NuSTAR (Nuclear Spectroscopic Telescope Array) mission has pinpointed an object responsible for this high-energy radiation.

The object, called Swift J0042.6+4112, is a possible pulsar, the dense remnant of a dead star that is highly magnetized and spinning, researchers say. This interpretation is based on its emission in high-energy X-rays, which NuSTAR is uniquely capable of measuring. The object’s spectrum is very similar to known pulsars in the Milky Way.

It is likely in a binary system, in which material from a stellar companion gets pulled onto the pulsar, spewing high-energy radiation as the material heats up.

"We didn't know what it was until we looked at it with NuSTAR," said Mihoko Yukita, lead author of a study about the object, based at Johns Hopkins University in Baltimore. The study is published in The Astrophysical Journal.

This candidate pulsar is shown as a blue dot in a NuSTAR X-ray image of Andromeda (also called M31), where the color blue is chosen to represent the highest-energy X-rays. It appears brighter in high-energy X-rays than anything else in the galaxy.

Read more ~ NASA.gov

Image: NASA's Nuclear Spectroscope Telescope Array, or NuSTAR, has identified a candidate pulsar in Andromeda -- the nearest large galaxy to the Milky Way. This likely pulsar is brighter at high energies than the Andromeda galaxy's entire black hole population.The inset image shows the pulsar candidate in blue, as seen in X-ray light by NuSTAR. The background image of Andromeda was taken by NASA's Galaxy Evolution Explorer in ultraviolet light. Andromeda is a spiral galaxy like our Milky Way but larger in size. It lies 2.5 million light-years away in the Andromeda constellation.     Credits: NASA/JPL-Caltech/GSFC/JHU

Solving The Andromeda Galaxy's Bright Mystery

New Post has been published on https://myupdatesystems.com/solving-the-andromeda-galaxys-bright-mystery/

Solving The Andromeda Galaxy's Bright Mystery

Our Milky Way’s closest large galactic neighbor, the spiral Andromeda galaxy, has a strange, and very well-kept secret that it has long successfully hidden from the prying eyes of curious astronomers. Andromeda features a powerful source of high-energy X-ray emission, but its identity has remained an intriguing mystery–until now. In March 2017, a team of astronomers reported in a new study that NASA’s Nuclear Spectroscopic Telescope Array (NuSTAR) mission has managed to detect the elusive object that is the culprit behind this high-energy radiation. The object, called Swift J0042.5+4112 is a possible pulsar–a newborn neutron star that is the extremely dense, city-sized corpse of a doomed massive star that has perished in a fiery, brilliant, and beautiful supernova blast. Born spinning wildly, as they emerge–much like the Phoenix Bird of Greek mythology–from the raging funeral pyre of their massive progenitor stars, pulsars are highly magnetized objects, and Swift J0042.6+4112 shows a spectrum that is very similar to known pulsars inhabiting our own Milky Way Galaxy.

This new interpretation of the identity of the mysterious object, haunting Andromeda, is based on its emission in high-energy X-rays, which NuSTAR is uniquely capable of measuring. Furthermore, Swift J0042.6+4112 is likely a binary system, in which material from a companion star gets ripped up by the vampire-like pulsar–which spews out high-energy radiation as the stolen material grows hotter, and hotter, and hotter.

“We didn’t know what it was until we looked at it with NuSTAR,” commented Dr. Mihoko Yukita in March 23, 2017, NASA Jet Propulsion Laboratory (JPL) Press Release. Dr. Yukita, who is of Johns Hopkins University in Baltimore, Maryland, is the lead author of a research paper, describing the mysterious object, that is published in the March 15, 2017, issue of The Astrophysical Journal. The JPL is in Pasadena, California.

This newly discovered possible pulsar reveals its presence as a blue dot in a NuSTAR image of the Andromeda Galaxy (M31). The color blue was chosen to represent the highest-energy X-rays. The pulsar candidate shows itself to be brighter than anything else in its host galaxy.

Neutron stars are Tokyo-sized stellar ghosts, and pulsars are rapidly and regularly whirling newborn neutron stars. Stars, like people, do not live forever. When a massive star, that is still on the hydrogen-burning main sequence of the Hertzsprung-Russell Diagram of Stellar Evolution, grows old and has finally depleted its necessary supply of thermonuclear fuel, it reaches the inevitable end of the stellar road. The imploded mess, composed of what is left of the erstwhile hydrogen-burning massive star, creates from this wreckage a very dense core–which will become the lingering neutron star. During the explosive event, the progenitor star’s outer gaseous layers collapse toward the core–the neutron star–then violently rebound outward in the terrible, fierce fireworks of a supernova tantrum. The rapidly twirling baby neutron star–the pulsar–shoots out a brilliant beam of radiation into space. This beam is frequently likened to the brilliant, sweeping beacon of a lighthouse on Earth, and it can be observed by astronomers as pulses of radio waves and other forms of radiation.

Neutron stars can travel throughout our Universe as isolated bodies, or as members of a binary system in close contact with another still-“living” main-sequence star–or even with another stellar ghost, similar to itself. Neutron stars have also been observed embedded within bright and beautifully glowing supernova remnants. Some neutron stars even serve as the stellar parents of very unfortunate planets. Pulsar planets are hostile worlds that are mercilessly showered by a constant rain of radiation flowing out from the young (and deadly) neutron star. Indeed, the first batch of exoplanets, discovered back in 1992, orbit a pulsar. Pulsars famously flicker brilliantly off and on with remarkable regularity The pulsations of these spinning objects occur because of their extremely rapid and regular rotation. Dr. Jocelyn Bell Burnell discovered the first pulsar in 1967 when she was still a graduate student at the University of Cambridge in the UK.

Stars are immense spheres of searing-hot, roiling, glaring gas. These brilliant balls of fire are pulled together very tightly by the relentless tug of their own powerful gravity. This is why the cores of stars are both extremely dense as well as extremely bright. In fact, stars are so hot that they can engage in the process of nuclear fusion–and it is this very process that lights their fires. Nuclear fusion causes the atoms of lighter elements–such as hydrogen and helium–to fuse together to form increasingly heavier and heavier atomic elements. The production of heavier atomic elements, within the cores of stars, is called stellar nucleosynthesis. Stellar nucleosynthesis starts with the fusion of hydrogen atoms. Hydrogen is both the most abundant and lightest atomic element in the Universe. The extremely hot cores of stars fuse hydrogen atoms into the second-lightest atomic element in the Universe–which is helium. Atomic elements heavier than helium are termed metals by astronomers. All of the metals were formed in the cores of seething hot stars–or, alternatively, in the supernova explosion that ends the life of a massive star. The heaviest atomic elements of all–such as gold and uranium–are fused in the supernova explosion (supernova nucleosynthesis).

Nuclear fusion churns out a large amount of energy, which is why stars are both hot and bright. This energy production results in radiation pressure that push everything out and away from the star. This pressure is powerful enough to maintain a very necessary balance because the relentless pull of gravity squeezes everything in. Radiation pressure and gravity are in a constant tug-of-war within the star. The battle continues until the star finally has managed to burn its necessary supply of nuclear fuel. At this very critical stage, gravity goes on to win the war. As a result of gravity’s victory, the star’s core implodes–and it goes supernova. This very delicate balance between gravity and radiation pressure is dependent on the mass of the star, with the most massive stars being squeezed much more tightly than their less massive skin. Because, in massive stars, the squeeze of their own gravity is so intense, their nuclear fusion reactions proceed much more quickly than in smaller stars. Massive stars live fast and die young. Less massive stars can live quietly and peacefully, for a very long time, before they finally perish.

The weird stellar corpses that are neutron stars are commonly only about 20 kilometers in diameter. However, they weigh-in at about 1.4 times that of our Sun. Indeed, one teaspoon full of neutron star material can weigh as much as a herd of buffalo. These hot, dense, and relatively small spheres have magnetic fields that are about 1,000,000 times more intense than the most powerful magnetic fields on Earth.

The collapsing iron core belonging to a doomed massive star–that is just about ready to go supernova–triggers a chaotic, violent, brilliant event. An iron core marks a massive star’s grand finale in the universal drama. This is because iron cannot serve as fuel in the process of nuclear fusion–and nuclear fusion is what has kept the erstwhile main-sequence star fluffy against the terrible squeeze of its own gravity.

Andromeda

Spiral galaxies like our large Milky Way, and the nearby Andromeda, are majestic, starlit pinwheels twirling elegantly in Space. Both our Milky Way and Andromeda are the two largest inhabitants of the Local Group of galaxies, which also hosts about 40 smaller galactic constituents. The Local Group is a few million light-years across. However, this is actually a small region when compared to immense galaxy clusters. Enormous galactic clusters can host literally hundreds of resident galaxies. Our own Local Group is situated near the outer limits of the Virgo Galaxy Cluster whose core is about 50 million light-years from us. The numerous groups of galaxies and galaxy clusters are themselves smaller denizens of the unimaginably immense web-like, heavy filaments, and slender broad expanses, that compose the Cosmic Web. For example, the so-called Great Wall is a sheet-like collection of galaxies situated approximately 200 million light-years away from us, and a similar enormous structure is named the Great Attractor. The Great Attractor is exerting a powerful gravitational pull on the entire Virgo Cluster of galaxies. We are, of course, carried away with the rest of the galactic inhabitants of the Local Group at the breathtaking speed of several hundred kilometers per second.

Right now, Andromeda is a safe 2 million light-years away from our Galaxy–but this will change. Unfortunately, gravity’s powerful grip is pulling Andromeda towards our Milky Way at about 100 kilometers per second–and the two large spirals are headed for a violent smash-up. The good news is that this fatal collision will not happen for about 4 billion years–but when it does, both our Milky Way and Andromeda will experience a sea-change, merging together to create an elliptical (football-shaped) single galaxy–replacing the duo of former elegant and lovely spirals. The new elliptical galaxy will be twice the size of the two spirals that went into its construction. The new galaxy, that will form from the wreckage, has been given the playful name of the Milkomeda Galaxy by astronomers–in honor of the duo of former spirals that will merge together to create it.

Solving The Andromeda Galaxy’s Bright Mystery

The new study uses numerous different observations of the mysterious, bright, and bewildering object dancing in Andromeda. The observations of this intriguing object were derived from various spacecraft. In 2013, NASA’s Swift satellite reported it as a high-energy source, but its classification was unknown. This is because there are numerous objects emitting low energy X-rays in that particular region.

It turned out that the lower-energy X-ray emission from the object was a source first detected back in the 1970s by NASA’s Einstein Observatory. Other spacecraft, such as the European Space Agency’s (ESA’s) XMM-Newton and NASA’s Chandra X-ray Observatory had also spotted it. However, it wasn’t until the more recent observations from NuSTAR–along with help derived from Swift satellite data–that astronomers realized that it was the same object as the probable pulsar that emits the high-energy X-ray light of Andromeda.

Astronomers have long thought that voracious black holes, which are more massive than pulsars, usually dominate the high-energy X-ray light in galaxies. As a delectable banquet of shredded stars and clouds of gas spiral down, down, down into the greedy gravitational grip of the hungry black hole–forming a bright structure surrounding it called an accretion disk–this unfortunate material gets hotter and hotter and hotter, and these extremely high temperatures emit high-energy radiation. The pulsar, which sports a lower mass than any of Andromeda’s resident black holes, is brighter at high energies than the galaxy’s entire black hole population.

Even the supermassive black hole lurking within Andromeda’s center does not possess significant high-energy X-ray emission associated with it. Therefore, it is puzzling how a solitary pulsar could be responsible for dominating Andromeda in high-energy X-ray light. Supermassive black holes are thought to lurk hungrily in the hearts of probably every large galaxy in the Universe–including our own–and they possess millions to billions of solar masses.

“NuSTAR has made us realize the general importance of pulsar systems as X-ray-emitting components of galaxies, and the possibility that the high-energy X-ray light of Andromeda is dominated by a single pulsar system only adds to this emerging picture,” Dr. Ann Hornschemeier explained in the March 23, 2017, JPL Press Release.

Un unique pulsar domine toute l'émission X de la galaxie d'Andromède

La source de rayons X qui domine toute la galaxie d'Andromède vient d'être identifiée, il s'agirait d'un seul et unique pulsar, nommé  Swift J0042.6+4112. Cette mise en évidence a été effectuée avec le télescope spatial NuSTAR. 

J0042.6 semble bien être un pulsar dans un système binaire, de ceux dont le pulsar accrète de la matière à son étoile compagne, jusqu'à former un disque de gaz fortement échauffé qui rayonne donc en rayons X. Son spectre en rayons X mesuré par NuSTAR est en tous cas très similaire à celui d'un tel système.

Mihoko Yukita, l'auteur de cette étude, résume : "Nous ne savions pas ce qu'était cette source X avant que nous l'observions avec NuSTAR". Il faut dire que l'existence de cette source X intense était connue depuis longtemps, même si sa nature était encore inconnue. C'est dans les années 1970 qu'elle a été détectée pour la première fois dans les basses énergies de rayons X par le télescope spatial Einstein Observatory a proximité du centre de la galaxie d'Andromède. Depuis, d'autres télescopes spatiaux spécialisés dans la détection des rayons X l'ont également détectée à plus haute énergie, comme Chandra X-ray Observatory et XMM-Newton. Mais c'est grâce aux observations combinées de Swift en 2013 et de NuSTAR plus récemment, notamment grâce à la forme du spectre des rayons X, que les astrophysiciens sont enfin parvenus à comprendre l'origine des ces rayons X de haute énergie. A ces  énergies jusqu'à une vingtaine de kiloélectronvolts (keV), J0042.6 apparaît être l'objet le plus brillant de toute la galaxie M31. Yukita et ses collaborateurs publient leur étude dans The Astrophysical Journal. Ils montrent que la source de rayons X de basse énergie et la source de rayons X de haute énergie ne font qu'une. Le spectre montre bien deux composante avec une composante à haute énergie qui subit une coupure brutale vers 20 keV, typique des accrétions de pulsar. Malheureusement, les données ne permettent pas d'identifier de pulsation, ce qui apporterait une preuve directe de la nature de la source, mais d'autres observations, avec Hubble notamment, permettent d'exclure la présence d'un objet compact de plus de 3 masses solaires. Or classiquement, les astronomes estiment que des rayons X d'aussi haute énergie ne peuvent qu'être produit par un disque d'accrétion de trou noir massif. Mais ici, la masse impliquée serait trop faible pour être ce genre de trou noir, et c'est donc l'hypothèse pulsar qui a les préférences de Yukita et son équipe.

D'ailleurs ce pulsar montre une luminosité à haute énergie qui est supérieure à celle de tous les trous noirs de la galaxie d'Andromède, y compris le trou noir supermassif de la galaxie, qui ne montre pas d'émission X aussi intense. Cette très grande luminosité de J0042.6 est inattendue. Le fait qu'un seul pulsar peut dominer à lui seul l'émission X à haute énergie d'une galaxie entière montre combien ces systèmes binaires ont une importance dans les galaxies.

Il est d'autant plus intéressant d'observer une telle source dans notre galaxie voisine qu'est la galaxie d'Andromède car elle est très similaire à notre galaxie. Observer Andromède est un moyen indirect (et plus aisé) d'étudier notre propre galaxie. Notre galaxie possède-t-elle elle aussi une source intense de rayons X de haute énergie ? Il semble que non pour le moment, mais on n'est jamais sûr de rien.

Référence

Identification of the Hard X-Ray Source Dominating the E > 25 keV Emission of the Nearby Galaxy M31 M. Yukita et al. The Astrophysical Journal, Volume 838, Number 1 (22 march 2017) http://ift.tt/2nbPRRS

Illustration

Andromède imagée en UV, le zoom représente l'image de la source X produite par NUSTAR  (NASA/JPL-Caltech/GSFC/JHU). 

via http://ift.tt/2mwSBMF