Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-05-09
Astrophys.J. 596 (2003) 437-450
Astronomy and Astrophysics
Astrophysics
Replaced with version accepted by ApJ. 40 pages, 8 figures
Scientific paper
10.1086/377628
We search for nearby, isolated, accreting, ``stellar-mass'' (3 to $100M_\odot$) black holes. Models suggest a synchrotron spectrum in visible wavelengths and some emission in X-ray wavelengths. Of 3.7 million objects in the Sloan Digital Sky Survey Early Data Release, about 150,000 objects have colors and properties consistent with such a spectrum, and 87 of these objects are X-ray sources from the ROSAT All Sky Survey. Thirty-two of these have been confirmed not to be black-holes using optical spectra. We give the positions and colors of these 55 black-hole candidates, and quantitatively rank them on their likelihood to be black holes. We discuss uncertainties the expected number of sources, and the contribution of blackholes to local dark matter.
Chisholm James R.
Dodelson Scott
Kolb Edward W.
No associations
LandOfFree
Stellar-Mass Black Holes in the Solar Neighborhood does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Stellar-Mass Black Holes in the Solar Neighborhood, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar-Mass Black Holes in the Solar Neighborhood will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-4290