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相关论文: X-ray and optical observations of M55 and NGC 6366…

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This paper is the first of a series dedicated to the X-ray properties of the young open cluster NGC 6231. Our data set relies on an XMM-Newton campaign of a nominal duration of 180 ks and reveals that NGC 6231 is very rich in the X-ray…

天体物理学 · 物理学 2009-11-11 H. Sana , E. Gosset , G. Rauw , H. Sung , J. -M. Vreux

This paper presents the analysis of candidate quiescent low mass xray binarie (qLMXBs) observed during a short Chandra/ACIS observation of the globular cluster (GC) NGC 6304. Two out of the three candidate qLMXBs of this cluster, XMMU…

星系天体物理 · 物理学 2009-07-22 S. Guillot , R. E. Rutledge , E. F. Brown , G. G. Pavlov , V. E. Zavlin

We present six monitoring observations of the starburst galaxy NGC 2146 using the Chandra X-ray Observatory. We have detected 67 point sources in the 8'.7 x 8'.7 field of view of the ACIS-S detector. Six of these sources were Ultra-Luminous…

Using the Chandra ACIS-I instruments, we have carried out the deepest X-ray observation on a typical Galactic plane region at l 28.5 deg, where no discrete X-ray sources have been known previously. We have detected, as well as strong…

天体物理学 · 物理学 2016-11-03 K. Ebisawa , A. Bamba , H. Kaneda , Y. Maeda , A. Paizis , G. Sato , S. Yamauchi

We present the results of Chandra observations of off-nuclear X-ray sources in the spiral galaxy M51 (NGC 5194). 113 X-ray sources have been detected in the field of view and 84 among them project within the disk of NGC 5194. Six and twenty…

天体物理学 · 物理学 2007-05-23 Yuichi Terashima , Andrew S. Wilson

Recent surveys of the Local Group spiral Galaxies M31 and M33 with XMM-Newton yielded a large number of X-ray sources. As part of the effort to identify and classify the objects responsible for this X-ray emission, we have obtained optical…

天体物理学 · 物理学 2009-11-11 D. Hatzidimitriou , W. Pietsch , Z. Misanovic , P. Reig , F. Haberl

X-ray binaries provide exceptional laboratories for understanding the physics of matter under the most extreme conditions. Until recently, there were few, if any, observational constraints on the circumbinary environments of X-ray binaries…

We have studied the X-ray source population of the face-on spiral galaxy M101 (NGC 5457). Within a field of radius 17' (36 kpc at the distance of 7.2 Mpc), covered by an ultradeep (229 ks) ROSAT HRI image, 51 X-ray sources are detected with…

天体物理学 · 物理学 2016-08-30 Q. Daniel Wang , Stefan Immler , Wolfgang Pietsch

Based on the archival data from the Chandra observations of nearby galaxies, we study different sub populations of low-mass X-ray binaries (LMXBs) - dynamically formed systems in globular clusters (GCs) and in the nucleus of M31 and…

We present the results of a 17 ks Chandra observation of the nearby dwarf spiral galaxy NGC 4395, focusing on the X-ray properties of the moderate-mass black hole that resides in its nucleus. Chandra affords the first high-quality,…

天体物理学 · 物理学 2007-05-23 E. C. Moran , M. Eracleous , K. M. Leighly , G. Chartas , A. V. Filippenko , L. C. Ho , P. R. Blanco

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

We report the discovery of an X-ray source coincident with the nuclear star cluster at the dynamical center of the nearby late-type spiral galaxy NGC 2403. The X-ray luminosity of this source varies from below detection levels, ~1e35 erg/s…

天体物理学 · 物理学 2011-02-11 Mihoko Yukita , Douglas A. Swartz , Roberto Soria , Allyn F. Tennant

A 90 ks Chandra HETG observation of the young stellar cluster NGC 6193 in the southern Ara OB1 association detected 43 X-ray sources in a 2' x 2' core region centered on the young O stars HD 150135 (O6.5V) and HD 150136 (O3+O6V). The…

天体物理学 · 物理学 2009-11-11 S. L. Skinner , S. A. Zhekov , F. Palla , C. L. D. R Barbosa

The Cartwheel is one of the most outstanding examples of a dynamically perturbed galaxy where star formation is occurring inside the ring--like structure. In previous studies with Chandra, we detected 16 Ultra Luminous X-ray sources lying…

天体物理学 · 物理学 2015-06-24 A. Wolter , G. Trinchieri , M. Colpi

We present a Chandra ACIS study of the early-type galaxy NGC 4552. We detect 47 X-ray point sources, most of which are likely LMXBs, within 4 R_e. The brightest X-ray source coincides with the optical/UV/radio center of the galaxy, and…

天体物理学 · 物理学 2009-11-11 Yueheng Xu , Haiguang Xu , Zhongli Zhang , Arunav Kundu , Yu Wang , Xiang-Ping Wu

Our campaign of deep monitoring observations with {\it Chandra} of the nearby elliptical galaxy NGC 3379 has lead to the detection of nine globular cluster (GC) and 53 field low mass X-ray binaries (LMXBs) in the joint {\it Hubble}/{\it…

We have discovered with XMM-Newton an X-ray source in the core of the globular cluster M13, whose X-ray spectral properties suggest that it is a quiescent neutron star X-ray binary. The spectrum can be well fitted with a pure hydrogen…

天体物理学 · 物理学 2011-05-23 Bruce Gendre , Didier Barret , Natalie A. Webb

We report the outbursts from a newly discovered X-ray transient in the Magellanic-type, SB(s)m galaxy NGC 55. The transient source, XMMU J001446.81-391123.48, was undetectable in the 2001 \xmm{} and 2004 \chandra{} observations, but…

高能天体物理现象 · 物理学 2015-02-26 V. Jithesh , Zhongxiang Wang

We report the detailed analysis of the X-ray properties of the discrete sources detected in a long (72 ks) \chandra ACIS-S observation of the Antennae galaxies. We detect 49 sources, down to a detection limit of ~ 10^{38} erg\s; 18 sources…

天体物理学 · 物理学 2009-11-07 A. Zezas , G. Fabbiano , A. H. Rots , S. S. Murray

We present results from a study of 2-8 keV X-ray sources detected by the Advanced CCD Imaging Spectrometer (ACIS) instrument on the Chandra X-ray Observatory in the field of the z=0.516 cluster CRSS J0030.5+2618. In our 63.5 arcmin^2 search…