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Related papers: Three LINERs Under the Chandra X-Ray Microscope

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We present a study of the X-ray emission from the nuclei of galaxies observed in the core of the Perseus cluster in a deep exposure with Chandra. Point sources are found coincident with the nuclei of 13 early-type galaxies, as well as the…

Astrophysics · Physics 2009-11-13 S. Santra , J. S. Sanders , A. C. Fabian

We present a spectral investigation of X-ray binaries in NGC 5128 (Cen A), using six 100 ks Chandra observations taken over two months in 2007. We divide our sample into thermally and non-thermally dominated states based on the behavior of…

We present the results of a study of discrete X-ray sources in NGC 6946 using a deep Chandra ACIS observation. Based on the slope of the log N-log S distribution and the general correlation of sources with the spiral arms, we infer that the…

Astrophysics · Physics 2009-11-07 S. S. Holt , E. M. Schlegel , U. Hwang , R. Petre

We present results from a 25 ksec CHANDRA ACIS-S observation of galaxies NGC4438 and NGC4435 in the Virgo Cluster. X-ray emission in NGC4438 is observed in a ~700 pc nuclear region, a 2.3 kpc spherical bulge, and a network of filaments…

Astrophysics · Physics 2009-11-10 Marie E. Machacek , Christine Jones , William R. Forman

We discuss ROSAT HRI X-ray observations of 33 very nearby galaxies, sensitive to X-ray sources down to a luminosity of approximately 10^38 erg/s. The galaxies are selected from a complete, volume limited sample of 46 galaxies with d<7 Mpc…

Astrophysics · Physics 2009-10-31 P. Lira , A. Lawrence , R. A. Johnson

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…

Recent Chandra observations have revealed a large population of faint X-ray point sources in the Galactic Centre. The observed population consists of about 2000 faint sources in the luminosity range ~10^31-10^33 erg/s. The majority of these…

Astrophysics · Physics 2009-11-13 A. J. Ruiter , K. Belczynski , T. E. Harrison

We present the results of the optical identifications of a set of X-ray sources from the all-sky surveys of INTEGRAL and SWIFT observatories. Optical data were obtained with Russian-Turkish 1.5-m Telescope (RTT150). Nine X-ray sources were…

Stellar archeology of nearby LINER galaxies may reveal if there is a stellar young population that may be responsible for the LINER phenomenon. We show results for the classical LINER galaxies NGC 4579 and NGC 4736 and find no evidence of…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 J. E. Steiner , R. B. Menezes , T. V. Ricci , A. S. Oliveira

Since the discovery of low-ionization nuclear emission-line regions in many galaxies (LINERs), it has been recognized that they constitute a class of active galactic nuclei (AGNs) which are thought to be powered by gas accretion onto a…

Astrophysics · Physics 2009-10-31 Yoshiaki Taniguchi , Yasuhiro Shioya , Takashi Murayama

Multi-epoch Chandra X-ray observations of nearby massive early-type galaxies open up the study of an important regime of low-mass X-ray binary (LMXB) behavior -- long term variability. In a companion paper, we report on the detection of 158…

We present the first results of the Chandra and optical follow-up observations of hard X-ray sources detected in the ASCA Medium Sensitivity Survey (AMSS). Optical identifications are made for five objects. Three of them show either weak or…

We analyze HST spectra and Chandra observations of a sample of 21 LINERs, at least 18 of which genuine AGN. We find a correlation between the X-rays and emission lines luminosities, extending over three orders of magnitude and with a…

Astrophysics of Galaxies · Physics 2015-07-02 Barbara Balmaverde , Alessandro Capetti

We report the detection of an absorbed central X-ray source and its strong, rapid variability in NGC4395, the least luminous Seyfert nucleus known. The X-ray source exhibits a number of flares with factors of 3-4 flux changes during a half…

Astrophysics · Physics 2009-09-17 K. Iwasawa , A. C. Fabian , O. Almaini , P. Lira , A. Lawrence , K. Hayashida , H. Inoue

We present X-ray observations of nine Weak-Line Radio Galaxies (WLRGs), optically classified as confirmed or possible Low Ionization Nuclear Emission-line Regions (LINERs). The data were taken from the Chandra, XMM, and BeppoSax archives.…

Astrophysics · Physics 2009-11-10 Alexander S. Rinn , Rita M. Sambruna , Mario Gliozzi

Earlier observations of NGC 1808 in various wavebands (X-ray, optical, near-infrared, radio) provided evidence for the existence of either a starburst or a Seyfert 2 nucleus. We here present the results of multiwavelength XMM-Newton and…

We report the detection of a weak X-ray point source coincident with the nucleus of the bulgeless disk galaxy NGC 3621, recently discovered by Spitzer to display high ionization mid-infrared lines typically associated with AGN. These…

High Energy Astrophysical Phenomena · Physics 2009-07-24 M. Gliozzi , S. Satyapal , M. Eracleous , L. Titarchuk , C. C. Cheung

We report the results of a programme of dual-epoch Chandra ACIS-S observations of five ultraluminous X-ray sources (ULXs) in nearby spiral galaxies. All five ULXs are detected as unresolved, point-like X-ray sources by Chandra, though two…

Astrophysics · Physics 2009-11-10 T. P. Roberts , R. S. Warwick , M. J. Ward , M. R. Goad

We report the discovery of an extremely broad H-alpha emission line in the LINER nucleus of NGC 4579. From ground-based observations, the galaxy was previously known to contain a Type 1 nucleus with a broad H-alpha line of FWHM = 2300 km/s…

Astrophysics · Physics 2009-10-31 A. J. Barth , L. C. Ho , A. V. Filippenko , H. -W. Rix , W. L. W. Sargent

In order to determine whether unified models of active galactic nuclei apply to low-luminosity objects, we have undertaken a spectropolarimetric survey of of LINERs and Seyfert nuclei at the Keck Observatory. The 14 objects observed have a…

Astrophysics · Physics 2009-10-31 A. J. Barth , A. V. Filippenko , E. C. Moran
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