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相关论文: A Deep Chandra View of the NGC 404 Central Engine

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We report on the nuclear X-ray properties of the radio galaxy NGC 6251 observed with XMM-Newton. NGC 6251 is a well-known radio galaxy with intermediate FRI/II radio properties. It is optically classified as a Seyfert 2 and hosts a…

天体物理学 · 物理学 2009-11-10 M. Gliozzi , R. M. Sambruna , W. N. Brandt , R. Mushotzky , M. Eracleous

We present an analysis of six 12 um selected Seyfert 2 galaxies that have been reported to be unabsorbed in the X-ray. By comparing the luminosities of these galaxies in the mid-IR (12um), optical ([O III]) and hard X-ray (2-10 keV), we…

天体物理学 · 物理学 2009-11-13 Murray Brightman , Kirpal Nandra

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 are conducting a search for supermassive black holes (SMBHs) with masses below 10^7 M_sun by looking for signs of extremely low-level nuclear activity in nearby galaxies that are not known to be AGNs. Our survey has the following…

天体物理学 · 物理学 2009-11-13 Himel Ghosh , Smita Mathur , Fabrizio Fiore , Laura Ferrarese

We present the results of Chandra observations of the Cl1604 supercluster at z~0.9. The system is the largest structure mapped at redshifts approaching unity, containing at least eight spectroscopically confirmed galaxy clusters and groups.…

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…

天体物理学 · 物理学 2009-11-13 Q. Daniel Wang , Katherine E. Whitaker , Rosa Williams

We use three Chandra observations, totalling 134.3 ks, to constrain the dynamical motion of NGC1404 falling towards the dominant elliptical NGC1399 through the Fornax ICM. NGC1404's surface brightness profile shows a sharp edge \~8 kpc from…

天体物理学 · 物理学 2009-11-10 M. Machacek , A. Dosaj , W. Forman , C. Jones , M. Markevitch , A. Vikhlinin , A. Warmflash , R. Kraft

Using ROSAT, we have made the first deep X-ray observations of NGC 7331, discovering a nuclear X-ray source coincident with the previously determined radio and optical nuclear centers. Positions, luminosities, and fluxes of X-ray sources in…

天体物理学 · 物理学 2009-10-30 Christopher J. Stockdale , W. Romanishin , John J. Cowan

We present an analysis of the X-ray properties of the Magellanic-type galaxy NGC 55 based on two contiguous XMM-Newton observations. We detect a total of 137 X-ray sources in the field of view, 42 of which are located within the optical…

天体物理学 · 物理学 2009-11-11 A-M. Stobbart , T. P. Roberts , R. S. Warwick

We studied the colliding galaxy NGC 7714 with two XMM-Newton observations, six months apart. The galaxy contains two bright X-ray sources: we show that they have different physical nature. The off-nuclear source is an accreting compact…

天体物理学 · 物理学 2009-11-10 Roberto Soria , Christian Motch

We present results from Chandra observations of the 3C/FRI sample of low luminosity radio-galaxies. We detected a power-law nuclear component in 12 objects out of the 18 with available data. In 4 galaxies we detected nuclear X-ray…

天体物理学 · 物理学 2009-11-11 B. Balmaverde , A. Capetti , P. Grandi

We present {\it Gemini} longslit optical spectroscopy and VLA radio observations of the nuclear region of NGC 4178, a late-type bulgeless disk galaxy recently confirmed to host an AGN through infrared and X-ray observations. Our…

宇宙学与河外天体物理 · 物理学 2015-06-17 Nathan Secrest , Shobita Satyapal , Sean Moran , Teddy Cheung , Marcello Giroletti , Mario Gliozzi , Marcel Bergmann , Anil Seth

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

With the superb angular resolution of the Chandra Observatory, it is now possible to detect X-ray point sources, either embedded in galaxy clusters or along the cluster line of sight, which could not be resolved by previous instruments.…

天体物理学 · 物理学 2009-11-11 M. Branchesi , I. M. Gioia , C. Fanti , R. Fanti , N. Cappelluti

We present new Chandra X-ray Observatory and Hubble Space Telescope observations of eight optically selected broad-line AGN candidates in nearby dwarf galaxies ($z<0.055$). Including archival Chandra observations of three additional…

高能天体物理现象 · 物理学 2017-02-15 Vivienne F. Baldassare , Amy E. Reines , Elena Gallo , Jenny E. Greene

We use deep Chandra X-ray Observatory observations to examine the coronae of the two brightest cluster galaxies in the Coma cluster of galaxies, NGC 4874 and NGC 4889. We find that NGC 4889 hosts a central depression in X-ray surface…

星系天体物理 · 物理学 2014-03-05 J. S. Sanders , A. C. Fabian , M. Sun , E. Churazov , A. Simionescu , S. A. Walker , N. Werner

Using the Chandra Advanced CCD Imaging Spectrometer Imaging array (ACIS-I), we have carried out a deep hard X-ray observation of the Galactic plane region at (l,b) ~ (28.5, 0.0), where no discrete X-ray source had been reported previously.…

Chandra ACIS-I data of the molecular cloud and HII region complex NGC 6334 were analyzed. The hard X-ray clumps detected with ASCA (Sekimoto et al. 2000) were resolved into 792 point sources. After removing the point sources, an extended…

天体物理学 · 物理学 2009-11-13 Yuichiro Ezoe , Motohide Kokubun , Kazuo Makishima , Yutaro Sekimoto , Keiichi Matsuzaki

A Chandra ACIS-S imaging observation of the nearby galaxy M81 (NGC 3031) reveals 9 luminous soft X-ray sources. The local environments, X-ray spectral properties, and X-ray light curves of the sources are presented and discussed in the…

天体物理学 · 物理学 2009-11-07 Douglas Swartz , Kajal Ghosh , Valery Suleimanov , Allyn Tennant , Kinwah Wu

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
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