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相关论文: Monitoring the X-ray Variability of Bright X-ray S…

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We present X-ray and optical observations of a new transient X-ray source in M31 first detected 23-May-2004 at R.A.=00:43:09.940 +/- 0.65'', Dec.=41:23:32.49 +/- 0.66''. The X-ray lightcurve shows two peaks separated by several months,…

In this paper we investigate the X-ray spectra and X-ray spectral variability of compact X-ray sources for 3 Chandra observations of the Local Group galaxy M33. The observations are centered on the nucleus and the star forming region NGC…

天体物理学 · 物理学 2009-11-13 H. -J. Grimm , J. McDowell , A. Zezas , D. -W. Kim , G. Fabbiano

We present the results of a study of the variability of X-ray sources in the central 30' of the nearby Andromeda Galaxy (M31) based on XMM Performance Verification observations. Two observations of this field, with a total exposure time of…

We examined 134 Chandra observations of the population of X-ray sources associated with globular clusters (GCs) in the central region of M31. These are expected to be X-ray binary systems (XBs), consisting of a neutron star or black hole…

高能天体物理现象 · 物理学 2015-06-04 R. Barnard , M. Garcia , S. S. Murray

From October 1999 to August 2002, 45 transient X-ray sources were detected in M31 by Chandra and XMM-Newton. We have performed spectral analysis of all XMM-Newton and Chandra ACIS detections of these sources, as well as flux measurements of…

天体物理学 · 物理学 2009-11-11 Benjamin F. Williams , S. Naik , Michael R. Garcia , Paul J. Callanan

We present an extension to our XMM-Newton X-ray source catalogue of M 31, containing 39 newly found sources. In order to classify and identify more of the sources we search for X-ray time variability in XMM-Newton archival data of the M 31…

天体物理学 · 物理学 2009-11-13 H. Stiele , W. Pietsch , F. Haberl , M. Freyberg

We have created 0.3--10 keV, 13 year, unabsorbed luminosity lightcurves for 528 X-ray sources in the central 20' of M31. We have 174 Chandra observations spaced at ~1 month intervals thanks to our transient monitoring program, deeper…

高能天体物理现象 · 物理学 2015-06-17 R. Barnard , M. R. Garcia , F. Primini , Z. Li , F. Baganoff , S. S. Murray

All 63 discrete X-ray sources brighter than L_{\rm X} = 5x10^{36} erg/s in any of four XMM-Newton observations of the core of M31 were surveyed for time variability over time-scales of seconds to thousands of seconds, and for intensity…

天体物理学 · 物理学 2016-08-30 R. Barnard , U. Kolb , J. P. Osborne

We investigate the long-term variability exhibited by the X-ray point sources in the starburst galaxy M82. By combining 9 Chandra observations taken between 1999 and 2007, we detect 58 X-ray point sources within the D25 isophote of M82 down…

高能天体物理现象 · 物理学 2015-05-20 Yi-Kuan Chiang , Albert K. H. Kong

Multi-epoch Chandra X-ray observations of nearby massive early-type galaxies open up the study of an important regime of low-mass X-ray binary (LMXB) behavior -- long term variability. In a companion paper, we report on the detection of 158…

天体物理学 · 物理学 2008-06-05 Gregory R. Sivakoff , Andrés Jord'an , Adrienne M. Juett , Craig L. Sarazin , Jimmy A. Irwin

We carried out new observations of two fields in the northern ring of M31 with XMM-Newton with two exposures of 100 ks each and obtained a complete list of X-ray sources down to a sensitivity limit of ~7 x 10^34 erg s^-1 (0.5 - 2.0 keV).…

We have been monitoring M31 with HRC and ACIS onboard \chandra regularly in the past two years. By combining eight \chandra ACIS-I observations taken between 1999 to 2001, we have identified 204 X-ray sources within the central $\sim…

天体物理学 · 物理学 2007-05-23 A. K. H. Kong , M. R. Garcia , F. A. Primini , R. Di Stefano , S. S. Murray

In this paper we present the source list for 3 Chandra observations of the Local Group galaxy M33. The observations are centered on the nucleus and on the star forming region NGC 604. We detect a total of 261 sources in an area of \~0.2…

天体物理学 · 物理学 2009-11-11 H. -J. Grimm , J. McDowell , A. Zezas , D. -W. Kim , G. Fabbiano

We present new optical spectroscopy of 20 candidate counterparts of 17 X-ray sources in the direction of the M31 disc. By comparing the X-ray catalogue from the XMM-Newton survey of M31 with star catalogues from the Local Group Galaxy…

[Abridged] The central field of the Andromeda galaxy (M 31) has been monitored, using the Chandra HRC-I detector (about 0.1-10 keV energy range) from 2006 to 2012 with the main aim to detect X-rays from optical novae. We present a…

高能天体物理现象 · 物理学 2015-06-15 F. Hofmann , W. Pietsch , M. Henze , F. Haberl , R. Sturm , M. Della Valle , D. H. Hartmann , D. Hatzidimitriou

We presented the results of an analysis of four XMM-Newton observations of the starburst galaxy IC342 taken over a four-year span from 2001 to 2005, with an emphasis on investigating the long-term flux and spectral variability of the X-ray…

高能天体物理现象 · 物理学 2011-01-17 Daisy S. Y. Mak , Chun S. J. Pun , Albert K. H. Kong

We report on \chandra observations of the central region of M31. By combining eight \chandra ACIS-I observations taken between 1999 and 2001, we have identified 204 X-ray sources within the central $\sim 17'\times17'$ region of M31, with a…

天体物理学 · 物理学 2008-11-26 A. K. H. Kong , M. R. Garcia , F. A. Primini , S. S. Murray , R. Di Stefano , J. E. McClintock

The Chandra ACIS Survey of M33 (ChASeM33) has acquired 7 fields of ACIS data covering M33 with 200 ks of exposure in each field. A catalog from the first 10 months of data, along with archival Chandra observations dating back to the year…

(Abridged) We present the results of the systematic survey of X-ray sources in the central region of M31 using the data from XMM-Newton observations performed in the years 2000-2004. The spectral properties and variability of 123 bright…

天体物理学 · 物理学 2007-05-23 Sergey Trudolyubov , William Priedhorsky , France Cordova

Over the last ~5 years we have identified ~35 black hole candidates (BHCs) in M31 from their X-ray spectra. Our BHCs exhibited 0.3--10 keV spectra consistent with the X-ray binary (XB) hard state, at luminosities that are above the upper…

高能天体物理现象 · 物理学 2015-06-22 R. Barnard , M. R. Garcia , F. Primini , S. S. Murray
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