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相关论文: Serendipitous X-ray Sources in the Chandra HRC Fie…

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We present optical spectra and near-infrared imaging of a sample of serendipitous X-ray sources detected in the field of Chandra observations of the A2390 cluster of galaxies. The sources have 0.5-7 keV fluxes of 0.6-8 x 10^{-14} erg…

天体物理学 · 物理学 2009-09-17 C. S. Crawford , P. Gandhi , A. C. Fabian , R. J. Wilman , R. M. Johnstone , A. J. Barger , L. L. Cowie

[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 present results of a search for optical counterparts of X-ray sources in and toward the globular cluster Omega Centauri (NGC 5139) using the Advanced Camera for Surveys (ACS) on the Hubble Space Telescope. The ACS data consist of a…

太阳与恒星天体物理 · 物理学 2015-06-12 Adrienne M. Cool , Daryl Haggard , Tersi Arias , Michelle Brochmann , Jason Dorfman , April Gafford , Vivian White , Jay Anderson

We present a catalog of 9017 X-ray sources identified in Chandra observations of a 2 by 0.8 degree field around the Galactic center. We increase the number of known X-ray sources in the region by a factor of 2.5. The catalog incorporates…

We present followup optical g', r', and i', imaging and spectroscopy of serendipitous X-ray sources detected in 6 archival Chandra, images included in the Chandra, Multiwavelength Project (ChaMP). Of the 486 X-ray sources detected between…

Based on archival Chandra observations, we present a systematic timing survey of several hundred X-ray sources in M31, M81, and Centaurus A, mostly low-mass X-ray binaries (LXMBs), focusing on searching and characterizing aperiodic and…

高能天体物理现象 · 物理学 2025-12-16 Jiachang Zhang , Zhiyuan Li , Ziqian Hua , Tong Bao

The following is a progress report on the long-term coronal activity of Alpha Centauri A (HD128620: G2V) and B (HD128621: K1V). Since 2005, Chandra X-ray Observatory has carried out semiannual pointings on AB, mainly with the High…

太阳与恒星天体物理 · 物理学 2015-06-18 Thomas R. Ayres

We describe progress in a programme to study a sample of sources typical of those which contribute a large fraction of the hard X-ray background. The sources are selected from the fields of approximately 10 ks Chandra cluster observations…

天体物理学 · 物理学 2007-05-23 P. Gandhi , C. S. Crawford , A. C. Fabian , R. J. Wilman , R. M. Johnstone , A. J. Barger , L. L. Cowie

We report the discovery of eight X-ray sources with periodic variability in 487 ks of observations of the Galactic center with Chandra. The sources are identified from a sample of 285 objects detected with 100-4200 net counts. Their periods…

天体物理学 · 物理学 2009-11-10 M. P. Muno , F. K. Baganoff , M. W. Bautz , W. N. Brandt , G. P. Garmire , G. R. Ricker , ;

The 10 by 10 degrees region around dynamic center of our Galaxy is known to host a large number of bright X-ray sources, most of which are low mass binary systems. While high luminosity Z-sources are especially bright in the standard X-ray…

天体物理学 · 物理学 2007-05-23 E. Churazov , M. Gilfanov , R. Sunyaev , S. Kuznetsov

We present first results from five XMM-Newton observations of the binary system Alpha Centauri, which has been observed in snapshot like exposures of roughly two hours each during the last two years. In all our observations the X-ray…

天体物理学 · 物理学 2009-11-11 J. Robrade , J. H. M. M. Schmitt , F. Favata

Six x-ray point sources, with luminosities of $4 \times 10^{38} - 2 \times 10^{39} \rm ergs s^{-1}$ in the 0.4--7 keV band, were detected in Chandra observations of the spiral galaxy M100. One source is identified with supernova SN 1979C…

天体物理学 · 物理学 2009-11-06 Philip Kaaret

We report the discovery of a bright transient X-ray source, CXOU J132518.2-430304, towards Centaurus A (Cen A) using six new Chandra X-Ray Observatory observations in 2007 March--May. Between 2003 and 2007, its flux has increased by a…

We present comprehensive X-ray point source catalogs of NGC~55, NGC~2403, and NGC~4214 as part of the Chandra Local Volume Survey. The combined archival observations have effective exposure times of 56.5 ks, 190 ks, and 79 ks for NGC~55,…

We summarize results of a search for X-ray-emitting binary stars in the massive globular cluster Omega Centauri (NGC 5139) using Chandra and HST. ACIS-I imaging reveals 180 X-ray sources, of which we estimate that 45-70 are associated with…

星系天体物理 · 物理学 2015-05-20 Daryl Haggard , Adrienne M. Cool , Tersi Arias , Michelle B. Brochmann , Jay Anderson , Melvyn B. Davies

X-ray point sources in galaxies are dominated by X-ray binaries (XRBs) that are variables or transients and whether their variability would alter the X-ray luminosity functions (XLF) is still in debate. Here we report on NGC 7331 as an…

高能天体物理现象 · 物理学 2019-07-17 Ruolan Jin , Albert K. H. Kong

We present an 82 ksec Chandra ACIS-I observation of a large-scale hierarchical complex, which consists of various clusters/groups of galaxies and low-surface brightness X-ray emission at z = 0.247. This high-resolution {\sl Chandra}…

天体物理学 · 物理学 2009-11-10 Q. Daniel Wang , Frazer Owen , Michael Ledlow

We present a small sample of Chandra X-ray sources selected from the fields of ACIS observations which probe fluxes around the break in the hard band source counts. The targets of these fields include 9 nearby galaxy clusters, 1 distant…

天体物理学 · 物理学 2009-09-17 P. Gandhi , C. S. Crawford , A. C. Fabian , R. M. Johnstone

We present results of a Chandra observation of a field in NGC 2264. The observations were taken with the ACIS-I camera with an exposure time of 48.1 ks. We present a catalog of 263 sources, which includes X-ray luminosity, optical and…

About 2 million seconds of Chandra observing time have been devoted to the Galactic center (GC), including large-scale surveys and deep pointings. These observations have led to the detection of about 4000 discrete X-ray sources and the…

天体物理学 · 物理学 2009-11-11 Q. Daniel Wang
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