X-RAY AND RADIO VARIABILITY OF M31*, THE ANDROMEDA GALAXY NUCLEAR SUPERMASSIVE BLACK HOLE

We confirm our earlier tentative detection of M31* in X-rays and measure its light curve and spectrum. Observations in 2004-2005 find M31* rather quiescent in the X-ray and radio. However, X-ray observations in 2006-2007 show M31* to be highly variable at times. A separate variable X-ray source is f...

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Main Authors: Garcia, M. R., Hextall, Richard, Galache, Jose, Melia, Fulvio, Murray, Stephen S., Primini, F. A., Sjouwerman, Loránt O., Williams, Ben, Baganoff, Frederick K
其他作者: MIT Kavli Institute for Astrophysics and Space Research
格式: 文件
语言:en_US
出版: Institute of Physics/American Astronomical Society 2015
在线阅读:http://hdl.handle.net/1721.1/96091