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Related papers: Chandra X-ray Sources in M101

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We present a detailed analysis of XMM archival data of two Ultraluminous X-ray Sources (ULXs) in the nearby spiral galaxy NGC 1313: NGC 1313 X-1 and X-2. The spectral continuum of these sources was modeled with a soft thermal component plus…

Astrophysics · Physics 2009-11-11 R. Turolla , P. Mucciarelli , L. Zampieri , R. Falomo , M. Chieregato , A. Treves

We present the first results from 60ks of observations of Arp 220 using the ACIS-S instrument on Chandra. We report the detection of several sources near the galaxy's nucleus, including a point source with a hard spectrum that is coincident…

Astrophysics · Physics 2009-11-07 D. L. Clements , J. C. McDowell , S. Shaked , A. C. Baker , K. Borne , L. Colina , S. Lamb , C. Mundell

We have studied the face-on, barred spiral M83 (NGC 5236) with Chandra. Eighty-one point sources are detected (above 3.5-sigma) in the ACIS S3 image: 15 of them are within the inner 16 arcsec region (starburst nucleus, resolved for the…

Astrophysics · Physics 2007-05-23 Roberto Soria , Kinwah Wu

We study a Chandra X-ray Observatory ACIS-S observation of the Galactic globular clusterM12. With a 26 ks exposure time, we detect 6 X-ray sources inside the half-mass radius (2.16 arcminutes) of which two are inside the core radius (0.72…

High Energy Astrophysical Phenomena · Physics 2011-02-11 Ting-Ni Lu , Albert K. H. Kong , Cees Bassa , Frank Verbunt , Walter H. G. Lewin , Scott F. Anderson , David Pooley

We present Chandra observations of the enigmatic galaxy IRAS00317-2142, which is classified as a star-forming galaxy on the basis of the ionization level of its emission lines. However, a weak broad H\alpha wing and a high X-ray luminosity…

Astrophysics · Physics 2016-08-30 I. Georgantopoulos , A. Zezas , M. J. Ward

We present results of a search for supernova remnants (SNRs) in archival Chandra images of M33. We have identified X-ray SNRs by comparing the list of Chandra, X-ray sources in M33 with tabulations of SNR candidates identified from (1)…

We present an analysis of the X-ray properties of a sample of solar- and late-type field stars identified in the Chandra Cosmic Evolution Survey (COSMOS), a deep (160ks) and wide (0.9 deg2) extragalactic survey. The sample of 60 sources was…

Solar and Stellar Astrophysics · Physics 2015-05-20 Nicholas J. Wright , Jeremy J. Drake , Francesca Civano

[abridged] We present point-source catalogs for the 4Ms Chandra Deep Field-South (CDF-S), which is the deepest Chandra survey to date and covers an area of 464.5 arcmin^2. We provide a main source catalog, which contains 740 X-ray point…

We present a small sample of Chandra X-ray sources selected from the fields of ACIS observations which probe fluxes around the break in the hard band source counts. The targets of these fields include 9 nearby galaxy clusters, 1 distant…

Astrophysics · Physics 2009-09-17 P. Gandhi , C. S. Crawford , A. C. Fabian , R. M. Johnstone

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…

Solar and Stellar Astrophysics · Physics 2017-06-27 Phyllis M. Lugger , Haldan N. Cohn , Adrienne M. Cool , Craig O. Heinke , Jay Anderson

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…

High Energy Astrophysical Phenomena · Physics 2024-03-26 Gourav Kumawat , Craig O. Heinke , Haldan N. Cohn , Phyllis M. Lugger

We report on Chandra observations of 18 hard X-ray (>20 keV) sources discovered with the INTEGRAL satellite near the Galactic plane. For 14 of the INTEGRAL sources, we have uncovered one or two potential Chandra counterparts per source.…

High Energy Astrophysical Phenomena · Physics 2015-06-05 John A. Tomsick , Arash Bodaghee , Sylvain Chaty , Jerome Rodriguez , Farid Rahoui , Jules Halpern , Emrah Kalemci , Mehtap Ozbey Arabaci

We present Chandra observations of 18 spectroscopically selected quasars, already known to be X-ray weak from previous ROSAT observations. All the sources but one are detected by Chandra, and spectral analysis suggests that most of them are…

Astrophysics · Physics 2009-11-07 G. Risaliti , M. Elvis , R. Gilli , M. Salvati

Recent observations with the Chandra X-ray Observatory have provided us with the capability to discriminate point sources, such as the supermassive black hole Sgr A*, from the diffuse emission within the inner 10'' of the Galaxy. The hot…

Astrophysics · Physics 2009-11-10 Gabriel Rockefeller , Chris L. Fryer , Fulvio Melia , Michael S. Warren

We present X-ray and optical analysis of 188 AGN identified from 497 hard X-ray (f (2.0-8.0 keV) > 2.7x10^-15 erg cm^-2 s^-1) sources in 20 Chandra fields (1.5 deg^2) forming part of the Chandra Multi-wavelength Project. These medium depth…

Our neighbouring large spiral galaxy, the Andromeda galaxy (M 31 or NGC 224), is an ideal target to study the X-ray source population of a nearby galaxy. NuSTAR observed the central region of M 31 in 2015 and allows studying the population…

High Energy Astrophysical Phenomena · Physics 2018-02-01 H. Stiele , A. K. H. Kong

We present an X-ray study of our nearest starburst galaxy IC 10, based on XMM-Newton and Chandra observations. A list of 73 XMM-Newton and 28 Chandra detections of point-like X-ray sources in the field is provided; a substantial fraction of…

Astrophysics · Physics 2009-11-13 Q. Daniel Wang , Katherine E. Whitaker , Rosa Williams

We present a detailed case study of the diffuse X-ray and H-alpha emission in the halo of NGC 253, a nearby edge-on starburst galaxy driving a galactic superwind. The arcsecond spatial resolution of the Chandra ACIS instrument allows us to…

Astrophysics · Physics 2009-11-07 D. K. Strickland , T. M. Heckman , K. A. Weaver , C. G. Hoopes , M. Dahlem

We present an updated catalog of X-ray point sources in the inner 500$\arcsec$ ($\sim$20 parsec) of the Galactic Center (GC), where the {\it nuclear star cluster} (NSC) stands, based on a total of $\sim$4.5 Ms of {\it Chandra} observations…

High Energy Astrophysical Phenomena · Physics 2018-04-04 Zhenlin Zhu , Zhiyuan Li , Mark R. Morris

We present the X-ray point source population in the nearby Virgo elliptical galaxy NGC 4636 from 3 Chandra/ACIS observations, totaling 193 ks, taken over 3 years. Using wavelet decomposition, we detect 318 point sources. Here, we use a…

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