Starburst Galaxies emit more radiation than a million suns emit at all wavelengths

Ultra-luminous X-Ray Sources in Starburst Galaxies

The Antennae Galaxies are an example of a starburst galaxy occurring from the collision of NGC 4038/NGC 4039. (Credit: NASA/ESA)
The Antennae Galaxies are an example of a starburst galaxy occurring from the collision of NGC 4038/NGC 4039. (Credit: NASA/ESA)

Ultra-luminous X-ray sources (ULXs) are point sources in the sky that are so bright in X-rays that each emits more radiation than a million suns emit at all wavelengths. ULXs are rare. Most galaxies (including our own Milky Way) have none, and those galaxies that do host a ULX usually contain only one. ULXs are also mysterious objects. They can’t be normal stars because their huge luminosities should then tear them apart.

Most astronomers think that ULXs are black holes more than about ten solar masses in size (so-called intermediate mass black holes) that are accreting matter onto a surrounding disk and emitting X-rays. Bright X-ray emission is not unusual – the nuclei of galaxies also are bright X-ray emitters – but they are super-massive black holes, while ULXs are neither super-massive nor located in galactic nuclei.

An artist's rendition of one of the newly discovered SPIRE 'hot starburst' galaxies (credit: NASA/CXC/M.Weiss)
An artist’s rendition of one of the newly discovered SPIRE ‘hot starburst’ galaxies (credit: NASA/CXC/M.Weiss)

CFA astronomers Stefano Mineo and Andy Goulding and their colleagues used the Chandra X-ray Observatory to search for ULXs in a sample of seventeen luminous infrared galaxies that are exceptionally bright because of their extreme star formation activity. If star formation does signal the presence of ULXs, or even produce them, then these objects should have many. The team discovered fifty-three ULXs (with an uncertainty of about 30% ) among the 139 X-ray sources present in this sample.

An Ultraluminous X-ray Source (ULX) in the center of galaxy M82 that astronomers had thought was a black hole is really the brightest pulsar ever recorded. (Credit:  X-ray: NASA/CXC/Univ. of Toulouse/M. Bachetti; Optical: NOAO)
An Ultraluminous X-ray Source (ULX) in the center of galaxy M82 that astronomers had thought was a black hole is really the brightest pulsar ever recorded. (Credit:
X-ray: NASA/CXC/Univ. of Toulouse/M. Bachetti; Optical: NOAO)

They report, however, that this ULX figure is actually ten times smaller than would be expected if ULXs correlated with simple star formation activity. They offer several possible explanations for this deficiency, including a surfeit of elements heavier than helium in these galaxies (these elements can suppress the birth of black holes).

The galaxy NGC 1068, seen here in X-ray (red), optical (green) and radio (blue), is actively forming stars and contains three ultra-luminous X-ray sources ULXs. Astronomers investigating the connections between young stars and ULXs have completed a study of active star-forming galaxies and were surprised to find they are deficient in ULXs. (Credit: NASA/CXC/MIT/C.Canizares, D.Evans, Optical NASA/STScI, Radio NSF/NRAO/VLA)

But the most likely scenario, they argue, is that large amounts of gas in these galaxies are present and absorbing X-rays, with the result that many of the ULXs present are not detected. Their conclusion implies that deep X-ray surveys of galaxies must take absorbing gas into account when estimating their internal X-ray properties and how this radiation affects the galaxies’ properties and evolution.

 

Reference(s):

“A Deficit of Ultraluminous X-ray Sources in Luminous Infrared Galaxies,” W. Luangtip, T. P. Roberts, S. Mineo, B. D. Lehmer, D. M. Alexander, F. E. Jackson, A. D. Goulding and J. L. Fischer, MNRAS 446, 470, 2015

Credit: Smithsonian Astrophysical Observatory

Physics in the News

Thursday, September 4, 2014

New map locates Milky Way in neighborhood of 100,000 galaxies

A new map places the Milky Way (black dot) within a large supercluster of galaxies (white dots) by tracing the gravitational pull of galaxies toward one another. White filaments reveal the paths of galaxies moving toward a gravitational center in the new supercluster, dubbed "Laniakea." (Blue, low galaxy density; green, intermediate; red, high.) SDvision interactive visualization software by DP at CEA/Saclay, France)
A new map places the Milky Way (black dot) within a large supercluster of galaxies (white dots) by tracing the gravitational pull of galaxies toward one another. White filaments reveal the paths of galaxies moving toward a gravitational center in the new supercluster, dubbed “Laniakea.” (Blue, low galaxy density; green, intermediate; red, high.) (Credit: DP at CEA/Saclay, France)
via nationalgeographic

Small asteroid to safely pass close to Earth Sunday

via nasa

Researcher advances a new model for a cosmological enigma — dark matter

This three-dimensional map offers a first look at the web-like large-scale distribution of dark matter, an invisible form of matter that accounts for most of the Universe's imaginary mass. The map reveals a loose network of dark matter filaments, gradually collapsing under the relentless pull of gravity, and growing clumpier over time. The three axes of the box correspond to sky position (in right ascension and declination), and distance from the Earth increasing from left to right (as measured by cosmological redshift). Note how the clumping of the dark matter becomes more pronounced, moving right to left across the volume map, from the early Universe to the more recent Universe.
This three-dimensional map offers a first look at the web-like large-scale distribution of dark matter, an invisible form of matter that accounts for most of the Universe’s imaginary mass. The map reveals a loose network of dark matter filaments, gradually collapsing under the relentless pull of gravity, and growing clumpier over time. The three axes of the box correspond to sky position, and distance from the Earth increasing from left to right. Note how the clumping of the dark matter becomes more pronounced, moving right to left across the volume map, from the early Universe to the more recent Universe. (Credit: NASA/ESA/Richard Massey)
via ku.edu

Dark energy hunt gets weird

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Cosmologists have revealed intruiging new ways to probe the mystery of whether dark energy exists and how it might be accelerating the universe’s growth. (Credit: Picturegarden/Getty)
via newscientist

Watching ‘the clock’ at the LHC

As time ticks down to the restart of the Large Hadron Collider, scientists are making sure their detectors run like clockwork.Photo by Antonio Saba, CERN
As time ticks down to the restart of the Large Hadron Collider, scientists are making sure their detectors run like clockwork.  (Credit: Antonio Saba, CERN)
via symmetrymagazine

Mind-blowing science explained: Neutron stars “are basically atoms as big as mountains”

via salon

Ultracold atoms juggle spins with exceptional symmetry

Schematic representation of a spin-exchanging collision. Two atoms in different orbitals (blue and green) and different spin orientations (black arrows) collide. The two atoms exiting the collision have swapped their spins after interacting. Crucially, the process is independent of the two specific initial spin states. Credit: LMU-München / MPQ, Quantum Many Body Systems Division Read more at: http://phys.org
Schematic representation of a spin-exchanging collision. Two atoms in different orbitals (blue and green) and different spin orientations (black arrows) collide. The two atoms exiting the collision have swapped their spins after interacting. Crucially, the process is independent of the two specific initial spin states. (Credit: LMU-München / MPQ, Quantum Many Body Systems Division)
via phys.org

How the enormous mirrors on the world’s largest telescope are made

The Giant Magellan Telescope (GMT) is a ground-based extremely large telescope planned for completion in 2020.[5] It will consist of seven 8.4 m (27.6 ft) diameter primary segments,[6] with the resolving power of a 24.5 m (80.4 ft) primary mirror and collecting area equivalent to a 22.0 m (72.2 ft) one,[7] (which is about 368 square meters) (Credit: wiki, Tarantola)
via gizmodo

Cosmic forecast: Dark clouds will give way to sunshine

via phys.org

Do exoplanets transform between classes?

A new analysis suggests that hot super-Earths might be the skeletal remnants of hot Jupiters stripped of their atmospheres. The above image is an artist’s depiction of an early stage in the destruction of a hot Jupiter by its star. (Credit: NASA / GSFC / Reddy, S. Hall)
via skyandtelescope