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相关论文: A Chandra X-ray Study of NGC 1068: II. The Luminou…

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By analyzing the Chandra ACIS S3 data we studied the X-ray properties of the low-mass and high-mass X-ray binary populations in the nearby spiral galaxy NGC 5055. A total of 43 X-ray point sources were detected within the 2 effective radii,…

天体物理学 · 物理学 2009-11-13 Bing Luo , Jiyao Chen , Zhongli Zhang , Yu Wang , Jingying Wang , Haiguang Xu

We report sub arc-second resolution X-ray imaging-spectroscopy of the archetypal type 2 Seyfert galaxy NGC 1068 with the Chandra X-ray Observatory. The observations reveal the detailed structure and spectra of the 13 kpc-extent nebulosity…

天体物理学 · 物理学 2009-11-06 A. J. Young , A. S. Wilson , P. L. Shopbell

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 present the source catalog of a new Chandra ACIS-I observation of NGC 300 obtained as part of the Chandra Local Volume Survey. Our 63 ks exposure covers ~88% of the D25 isophote (R~6.3 kpc) and yields a catalog of 95 X-ray point sources…

We present the first results of an XMM-Newton EPIC observation of the luminous X-ray source population in the supergiant spiral galaxy M101. We have studied the properties of the fourteen most luminous sources, all of which have intrinsic…

天体物理学 · 物理学 2009-11-10 L. P. Jenkins , T. P. Roberts , R. S. Warwick , R. E. Kilgard , M. J. Ward

With a Chandra ACIS-S3 observation, we detect 42 X-ray point sources in the elliptical galaxy NGC 720, including a possible central source. Most of these sources will be low-mass X-ray binaries (LMXBs), and 12 are located within 2" of…

天体物理学 · 物理学 2009-11-07 Tesla E. Jeltema , Claude R. Canizares , David A. Buote , Gordon P. Garmire

In this paper we investigate the X-ray spectra and X-ray spectral variability of compact X-ray sources for 3 Chandra observations of the Local Group galaxy M33. The observations are centered on the nucleus and the star forming region NGC…

天体物理学 · 物理学 2009-11-13 H. -J. Grimm , J. McDowell , A. Zezas , D. -W. Kim , G. Fabbiano

We study the X-ray and optical properties of the ultraluminous X-ray source (ULX) X-6 in the nearby galaxy NGC 4258 (M106) based on the archival {\it XMM-Newton}, {\it Chandra}, {\it Swift}, and {\it Hubble Space Telescope} ({\it HST})…

高能天体物理现象 · 物理学 2016-09-22 Hasan Avdan , Senay Avdan , Aysun Akyuz , Solen Balman , Nazim Aksaker , Inci Akkaya Oralhan

We present a deep search for and analysis of X-ray sources in a sample of dwarf galaxies (M$_{r}$ < -15.5 mag) located within twelve galaxy clusters from the Kapteyn IAC WEAVE INT Cluster Survey (KIWICS) of photometric observations in the…

星系天体物理 · 物理学 2023-08-09 Şeyda Şen , Ersin Göğüş , Reynier F. Peletier , Nelvy Choque-Challapa , Amirnezam Amiri

We present a comprehensive X-ray point source catalog of NGC 404 obtained as part of the Chandra Local Volume Survey. A new, 97 ks Chandra ACIS-S observation of NGC 404 was combined with archival observations for a total exposure of ~123…

高能天体物理现象 · 物理学 2015-06-12 B. Binder , B. F. Williams , M. Eracleous , T. J. Gaetz , A. K. H. Kong , E. D. Skillman , D. R. Weisz

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

The advanced capabilities of the Chandra and XMM-Newton observatories mean that, for the first time, the detailed study of the brightest point-like X-ray sources in nearby galaxies outside of the local group is a realistic aim. Here, we…

天体物理学 · 物理学 2007-05-23 T. P. Roberts , M. R. Goad , M. J. Ward , R. S. Warwick , P. Lira

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

Despite the 30-year history of ultra-luminous X-ray sources (ULXs) studies, issues like the majority of their physical natures (i.e., neutron stars, stellar-mass black holes, or intermediate black holes) as well as the accretion mechanisms…

高能天体物理现象 · 物理学 2023-08-15 Chen-Hsun Ma , Kwan-Lok Li , You-Hua Chu , Albert K. H. Kong

In this paper we present the source list for 3 Chandra observations of the Local Group galaxy M33. The observations are centered on the nucleus and on the star forming region NGC 604. We detect a total of 261 sources in an area of \~0.2…

天体物理学 · 物理学 2009-11-11 H. -J. Grimm , J. McDowell , A. Zezas , D. -W. Kim , G. Fabbiano

[abridged] We investigate the nature of the luminous X-ray source population detected in a (72 ks) Chandra ACIS-S observation of NGC 4038/39, the Antennae galaxies. We derive the average X-ray spectral properties of sources in different…

天体物理学 · 物理学 2017-11-29 A. Zezas , G. Fabbiano , A. H. Rots , S. S. Murray

New HST observations show that the bright X-ray source in the face-on spiral galaxy NGC 1073 is located near a ring of recent star formation with an age of 8-16 Myr. This strengthens the association of X-ray sources in spiral galaxies…

天体物理学 · 物理学 2009-11-11 Philip Kaaret

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

ROSAT, and now Chandra, X-ray images allow studies of extranuclear X-ray point sources in galaxies other than our own. X-ray observations of normal galaxies with ROSAT and Chandra have revealed that off-nuclear, compact,…

天体物理学 · 物理学 2009-11-07 E. Colbert , A. Ptak

VLT images in $BVI$ are used to identify the optical counterparts to bright CHANDRA X-ray points sources discovered by Kraft et al. (2001, ApJ, 560, 675) in NGC5128. Of a total of 111 X-ray point sources with L_X>2*10^{36} ergs/s present in…

天体物理学 · 物理学 2009-11-10 Dante Minniti , Marina Rejkuba , Jose G. Funes S. J. , Sanae Akiyama
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