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相关论文: A Comprehensive Analysis of X-ray Sources in Terza…

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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 present a Chandra observation of the globular cluster Terzan 5 during times when the neutron-star X-ray transient EXO 1745-248 located in this cluster was in its quiescent state. We detected the quiescent system with a (0.5-10 keV)…

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…

We analyzed 1441 Chandra X-ray point sources in 32 nearby galaxies. The total point-source X-ray luminosity L_XP is well correlated with B, K, and FIR+UV luminosities of spiral host galaxies, and with the B and K luminosities for…

天体物理学 · 物理学 2011-05-05 Edward Colbert , Tim Heckman , Andy Ptak , Dave Strickland , Kim Weaver

Ultraluminous X-ray Sources (ULXs) in globular clusters are low mass X-ray binaries that achieve high X-ray luminosities through a currently uncertain accretion mechanism. Using archival Chandra and Hubble Space Telescope observations, we…

高能天体物理现象 · 物理学 2022-11-30 E. Thygesen , Y. Sun , J. Huang , K. C. Dage , S. E. Zepf , A. Kundu , D. Haggard , T. J. Maccarone

Based on archival {\it Chandra} data, we have carried out an X-ray survey of 69, or nearly half the known population of, Milky Way globular clusters (GCs), focusing on weak X-ray sources, mainly cataclysmic variables (CVs) and coronally…

高能天体物理现象 · 物理学 2018-05-16 Zhongqun Cheng , Zhiyuan Li , Xiaojie Xu , Xiangdong Li

The newly discovered 11 Hz accreting pulsar, IGR J17480-2446, located in the globular cluster Terzan 5, has shown several bursts with a recurrence time as short as few minutes. The source shows the shortest recurrence time ever observed…

高能天体物理现象 · 物理学 2015-05-27 S. Motta , A. D'Aì , A. Papitto , A. Riggio , T. Di Salvo , L. Burderi , T. Belloni L. Stella , R. Iaria

We combined Chandra ACIS observations of the globular cluster 47 Tucanae (hereafter, 47 Tuc) from 2000, 2002, and 2014-15 to create a deeper X-ray source list, and study some of the faint radio millisecond pulsars (MSPs) present in this…

We report on exploratory Chandra observations of five galactic nuclei that were found to be X-ray bright during the ROSAT all-sky survey (with L_X > 10^43 erg s^-1) but subsequently exhibited a dramatic decline in X-ray luminosity. Very…

天体物理学 · 物理学 2009-11-10 S. Vaughan , R. Edelson , R. S. Warwick

X-ray observations provide a unique probe of the accretion disk corona of supermassive black holes (SMBHs). In this paper, we present a uniform \emph{Chandra} X-ray data analysis of a sample of 152 $z\geq4.5$ quasars. We firmly detect 46…

高能天体物理现象 · 物理学 2021-05-26 Jiang-Tao Li , Feige Wang , Jinyi Yang , Joel N. Bregman , Xiaohui Fan , Yuchen Zhang

The ~1 Ms Chandra Deep Field North observation is used to study the extended X-ray sources in the region surrounding the Hubble Deep Field North (HDF-N), yielding the most sensitive probe of extended X-ray emission at cosmological distances…

The current generation of X-ray observatories like Chandra allows studies with very fine spatial details. It is now possible to resolve X-ray point sources projected into the cluster diffuse emission and exclude them from the analysis to…

天体物理学 · 物理学 2009-11-13 M. Branchesi , I. M. Gioia , C. Fanti , R. Fanti

We report on the Chandra ACIS-S3 imaging observation of the globular cluster NGC 6752. We detect 6 X-ray sources within the 10.5" core radius and 13 more within the 115" half-mass radius down to a limiting luminosity of Lx approx 10^{30}…

Over the past two years, we used a series of GBT observations to uncover at least 33 millisecond pulsars in the globular cluster Terzan 5 located in the Galactic bulge. We now have 32 timing solutions for the pulsars which give us precise…

天体物理学 · 物理学 2007-05-23 Scott M. Ransom

Presented here are the highlights from the deep Chandra observation of the elliptical galaxy NGC 3379. From the multi-epoch observation of this galaxy, 132 discrete X-ray sources have been detected within the region overlapped by all…

天体物理学 · 物理学 2007-12-24 N. J. Brassington

We present a survey of X-ray point sources in the nearest and dynamically young galaxy cluster, Virgo, using archival Chandra observations that sample the vicinity of 80 early-type member galaxies. The X-ray source populations at the…

星系天体物理 · 物理学 2017-09-20 Meicun Hou , Zhiyuan Li , Eric W. Peng , Chengze Liu

We analyse 55 ks of Chandra X-ray observations of the Galactic globular cluster M13. Using the latest radio timing positions of six known millisecond pulsars (MSPs) in M13 from Wang et al. (2020), we detect confident X-ray counterparts to…

高能天体物理现象 · 物理学 2021-01-27 Jiaqi Zhao , Yue Zhao , Craig O. Heinke

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

We present results from a Chandra X-ray Observatory study of the field X-ray source population in the vicinity of the radio galaxy MRC 1138-262. Many serendipitous X-ray sources are detected in an area of 8'x8' around the radio source and…

天体物理学 · 物理学 2009-11-07 L. Pentericci , J. D. Kurk , C. L. Carilli , D. E. Harris , G. K. Miley , H. J. A. Rottgering

We report on the population of point sources discovered during an 18.5 ksec Chandra ACIS-S observation of the Sombrero Galaxy. We present the luminosity function, the spectra of the 6 brightest sources, consider correlations with globular…

天体物理学 · 物理学 2009-11-10 R. Di Stefano , A. K. H. Kong , M. L. VanDalfsen , W. E. Harris , S. S. Murray , K. M. Delain
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