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相关论文: Identification of Faint Chandra X-ray Sources in t…

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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}…

We report the results of a deep search for faint Chandra X-ray sources, radio sources, and optical counterparts in the nearby, core-collapsed globular cluster, NGC 6752. We combined new and archival Chandra imaging to detect 51 X-ray…

We have searched for optical identifications for 79 Chandra X-ray sources that lie within the half-mass radius of the nearby, core-collapsed globular cluster NGC 6397, using deep Hubble Space Telescope Advanced Camera for Surveys Wide Field…

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 results of the Chandra deep imaging observation of the closest post-core collapse globular cluster, NGC 6397. Some 25 sources are detected within 2 arcmin of the cluster center of which about 20 are likely cluster members with L_x…

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

We analyse a Chandra observation of the rich globular cluster NGC 362, finding 33 X-ray sources within 1' (1.2 half-mass radii) of the cluster center. Spectral analysis of the brightest source (X1) shows blackbody-like emission, indicating…

高能天体物理现象 · 物理学 2024-03-26 Gourav Kumawat , Craig O. Heinke , Haldan N. Cohn , Phyllis M. Lugger

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 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

We present results of a search for objects with H-alpha excess, such as cataclysmic variables (CVs) and chromospherically active binaries (ABs), as counterparts to X-ray sources detected with Chandra satellite observatory in six Galactic…

星系天体物理 · 物理学 2009-10-08 Pawel Pietrukowicz

We present the results of a photometric survey for variable stars in the field of the nearby globular cluster NGC 6752. The cluster was monitored in 1996 and 1997 for a total of 54 hours with 3 different CCD cameras mounted on the 1.0-m…

天体物理学 · 物理学 2009-10-31 Ian B. Thompson , Janusz Kaluzny , Wojtek Pych , Wojtek Krzeminski

We report time-series photometry for 16 variable stars located in the central part of the globular cluster NGC 6752. The sample includes 13 newly identified objects. The precision of our differential photometry ranges from 1 mmag at V=14.0…

太阳与恒星天体物理 · 物理学 2014-11-20 Janusz Kaluzny , Ian B. Thompson

We present a deep ($\sim 330~\mathrm{ks}$) {\it Chandra} survey of the Galactic globular cluster M30 (NGC 7099). Combining the new Cycle 18 with the previous Cycle 3 observations we report a total of 10 new X-ray point sources within the…

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

Using the Hubble Ultraviolet Globular Cluster Survey (HUGS) and additional HST archival data, we have carried out a search for optical counterparts to the low-luminosity Chandra X-ray sources in the globular cluster M4 (NGC 6121). We have…

高能天体物理现象 · 物理学 2023-06-28 Phyllis M. Lugger , Haldan N. Cohn , Craig O. Heinke , Jiaqi Zhao , Yue Zhao , Jay Anderson

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 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

Highly sensitive and precise X-ray imaging from Chandra, combined with the superb spatial resolution of HST optical images, dramatically enhances our empirical understanding of compact binaries such as cataclysmic variables and low mass…

太阳与恒星天体物理 · 物理学 2015-05-20 Bruce Margon , B. Beck-Winchatz , L. Homer , D. Pooley , C. G. Bassa , S. F. Anderson , W. H. G. Lewin , F. Verbunt , A. K. H. Kong , R. M. Plotkin

We report on archival Hubble Space Telescope (HST) observations of the globular cluster M71 (NGC 6838). These observations, covering the core of the globular cluster, were performed by the Advanced Camera for Surveys (ACS) and the Wide…

太阳与恒星天体物理 · 物理学 2015-05-14 R. H. H. Huang , W. Becker , P. D. Edmonds , R. F. Elsner , C. O. Heinke , B. C. Hsieh

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

We present the results of a multi-wavelength (FUV to I-band) survey of the stellar populations of the globular cluster NGC 6752, using STIS, ACS and WFC3 on board the Hubble Space Telescope. We have confirmed that two previously identified…

太阳与恒星天体物理 · 物理学 2015-06-04 G. S. Thomson , C. Knigge , A. Dieball , T. J. Maccarone , A. Dolphin , D. Zurek , K. S. Long , M. Shara , A. Sarajedini
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