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相关论文: Chandra observations of the globular cluster M54

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We report our analysis of a Chandra X-ray observation of the rich globular cluster M80, in which we detect some 19 sources to a limiting 0.5-2.5 keV X-ray luminosity of 7*10^30 ergs/s within the half-mass radius. X-ray spectra indicate that…

天体物理学 · 物理学 2009-11-07 C. O. Heinke , J. E. Grindlay , P. D. Edmonds , D. A. Lloyd , S. S. Murray , H. N. Cohn , P. M. Lugger

We observed the nearby, low-density globular cluster M71 (NGC 6838) with the Chandra X-ray Observatory to study its faint X-ray populations. Five X-ray sources were found inside the cluster core radius, including the known eclipsing binary…

We have conducted Chandra observations of ~2560 square arcmin (~131 kpc^2) of of M31, and find that the most luminous X-ray sources in our fields are in globular clusters (GCs). Of the 28 GC X-ray sources in our fields, 17 are newly…

天体物理学 · 物理学 2016-08-30 R. Di Stefano , A. K. H. Kong , M. R. Garcia , P. Barmby , J. Greiner , S. S. Murray , F. A. Primini

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}…

(Abridged) We present the results of M31 globular cluster (GC) X-ray source survey, based on the data of XMM-Newton and Chandra observations covering ~6100 sq.arcmin of M31. We detected 43 X-ray sources coincident with globular cluster…

天体物理学 · 物理学 2008-11-26 Sergey Trudolyubov , William Priedhorsky

We report the detection of six discrete, low-luminosity (Lx < 10^33 erg/s) X-ray sources, located within 12 arcsec of the center of the collapsed-core globular cluster M30 (NGC 7099), and a total of 13 sources within the half-mass radius,…

We observed the globular cluster NGC 6652 with Chandra for 47.5 ks, detecting six known X-ray sources, as well as five previously undetected X-ray sources. Source A (XB 1832-330) is a well-known bright low-mass X-ray binary (LXMB). The…

高能天体物理现象 · 物理学 2015-06-04 W. S. Stacey , C. O. Heinke , H. N. Cohn , P. M. Lugger , A. Bahramian

As part of our campaign to determine the nature of the various source populations of the low-luminosity globular cluster X-ray sources, we have obtained a Chandra X-ray Observatory ACIS-S3 image of the globular cluster NGC 6440. We detect…

We report on the Chandra X-ray Observatory observations of the globular cluster NGC 288. We detect four X-ray sources within the core radius and seven additional sources within the half-mass radius down to a limiting luminosity of Lx=7e30…

天体物理学 · 物理学 2011-02-11 A. K. H. Kong , C. Bassa , D. Pooley , W. H. G. Lewin , L. Homer , F. Verbunt , S. F. Anderson , B. Margon

The globular cluster M15 was observed on three occasions with the High Resolution Camera on board Chandra in 2001 in order to investigate the X-ray source population in the cluster centre. After subtraction of the two bright central…

天体物理学 · 物理学 2009-11-10 D. C. Hannikainen , P. A. Charles , L. van Zyl , A. K. H. Kong , L. Homer , P. Hakala , T. Naylor , M. B. Davies

Using archival spectral-imaging data with a total exposure of $\sim144$ ks obtained by {\it Chandra}, 43 X-ray sources are detected within the half-light radius of globular cluster M62 (NGC6266). Based on the X-ray colour-luminosity diagram…

高能天体物理现象 · 物理学 2020-09-01 Kwangmin Oh , C. Y. Hui , K. L. Li , A. K. H. Kong

Using new Chandra X-ray observations and existing XMM-Newton X-ray and Hubble far ultraviolet observations, we aim to detect and identify the faint X-ray sources belonging to the Galactic globular cluster NGC 2808 in order to understand…

天体物理学 · 物理学 2009-11-13 M. Servillat , A. Dieball , N. A. Webb , C. Knigge , R. Cornelisse , D. Barret , K. S. Long , M. M. Shara , D. R. Zurek

We report a $30~\mathrm{ks}$ $Chandra$ ACIS-S survey of the globular cluster M3. Sixteen X-ray sources were detected within the half-light radius ($2.3'$) with $L_X \gtrsim 2.3 \times 10^{31}~\mathrm{erg~s^{-1}}$. We used…

高能天体物理现象 · 物理学 2018-12-14 Yue Zhao , Craig O. Heinke , Haldan N. Cohn , Phyillis M. Lugger , Adrienne M. Cool

We report here the results of the first Chandra X-Ray Observatory observations of the globular cluster M28 (NGC 6626). 46 X-ray sources are detected, of which 12 lie within one core radius of the center. We show that the apparently extended…

We present the results of two Chandra observations (separated by 1 year) of the population of X-ray sources in the spiral galaxy M51 (NGC 5194 and NGC 5195). 113 X-ray sources have been detected in an 8'.4x8'.4 region. Nine and 28 sources…

天体物理学 · 物理学 2009-11-07 Yuichi Terashima , Andrew S. Wilson

We report our analysis of a Chandra X-ray observation of the rich globular cluster Terzan 5, in which we detect 50 sources to a limiting 1.0-6 keV X-ray luminosity of 3*10^{31} ergs/s within the half-mass radius of the cluster. Thirty-three…

天体物理学 · 物理学 2008-11-26 C. O. Heinke , R. Wijnands , H. N. Cohn , P. M. Lugger , J. E. Grindlay , D. Pooley , W. H. G. Lewin

We have searched for optical identifications for 39 Chandra X-ray sources that lie within the 1.9 arcmin half-mass radius of the nearby (d = 4.0 kpc), core-collapsed globular cluster, NGC 6752, using deep Hubble Space Telescope ACS/WFC…

太阳与恒星天体物理 · 物理学 2017-06-27 Phyllis M. Lugger , Haldan N. Cohn , Adrienne M. Cool , Craig O. Heinke , Jay Anderson

We report on the Chandra X-ray Observatory ACIS-S3 imaging observation of the Galactic globular cluster M4 (NGC 6121). We detect 12 X-ray sources inside the core and 19 more within the cluster half-mass radius. The limiting luminosity of…

We report on a deep XMM-Newton EPIC observation of the globular cluster Omega Cen performed on August 13th, 2001. We have detected 11 and 27 faint X-ray sources in the core and half mass radii, searching down to a luminosity of 1.3 x…

天体物理学 · 物理学 2009-11-07 Bruce Gendre , Didier Barret , Natalie A. Webb

We have observed two low concentration Galactic globular clusters with the X-ray observatory XMM-Newton. We detect 47 faint X-ray sources in the direction of M 55 and 62 in the field of view of NGC 3201. Using the statistical Log N-Log S…

天体物理学 · 物理学 2009-11-11 N. A. Webb , P. J. Wheatley , D. Barret
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