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DSS Optical Image of M101
(Credit: Pal.Obs. DSS)

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NGC 4697
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Quasisoft Sources - Enigmatic X-ray Sources Point to Possible New Black Hole Population

Credit: NASA/CXC/SAO/R.DiStefano et al.

Chandra observations of the spiral galaxy M101 and several other nearby galaxies have revealed a possible new class of X-ray sources. These mysterious X-ray sources, marked with green diamonds in the image, are called "quasisoft" sources because they have a temperature in the range of one to four million degrees Celsius.

The power output of quasisoft sources is comparable to or greater than that of neutron stars or stellar-mass black holes fueled by the infall of matter from companion stars. This implies that the region that produces the X-rays in a quasisoft source is dozens of times larger.

One explanation is that these sources are produced by intermediate-mass black holes that have masses a hundred or more times greater than the mass of the Sun. Such objects would have much larger event horizons, which would account for the larger sizes and lower temperatures associated with the quasisoft sources. Alternatively, they could be standard neutron stars or stellar black holes where the associated region of hot gas is for some as yet unknown reason much larger than usual.



NGC 4697

"Hard" X-ray sources, such as neutron stars or stellar-mass black holes have temperatures greater than ten million degrees. The "supersoft" X-ray sources due to white dwarfs have temperatures of several hundred-thousand-degrees. A total of 72 quasisoft sources were discovered in the four galaxies: M101, M83, M51, and NGC 4697.

Until a few years ago, astronomers only knew of two sizes of black holes: stellar black holes with masses about ten times that of the Sun, and supermassive black holes located at the centers of galaxies, with masses ranging from millions to billions times that of the Sun. Recent evidence, however, suggests that a class of "intermediate-mass" black holes may also exist. Theories for the formation of intermediate-mass black holes involve the collapse of extremely massive stars, or the merger of many stellar-mass black holes.

As more quasisoft sources are discovered, the types of galaxies in which they reside and where they are located in a galaxy should give astronomers additional clues as to their nature and how they are formed. The present study indicates that quasisoft occur in various locations in elliptical as well as spiral galaxies.

Fast Facts for M101:
Credit  NASA/CXC/SAO/R.DiStefano et al.
Scale  Image is 14.0 arcmin across.
Category  Normal Galaxies & Starburst Galaxies
Coordinates (J2000)  RA 14h 03m 10.50s | Dec +54° 21’ 34.80"
Constellation  Ursa Major
Observation Dates  March 26, 2000
Observation Time  26 hours
Obs. IDs  934
Color Code  Energy (Red: 0.3-1.0 keV, Green: 1.0-2.0 keV, Blue: 2.0-8.0 keV)
Instrument  ACIS
Also Known As NGC 5457, The Pinwheel Galaxy
References R. DiStefano and A. Kong, astro-ph0311375
Distance Estimate  21 million light years
Release Date  March 01, 2004