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Related papers: X-ray properties of LINERs

200 papers

We present a systematic search for variability among the ROSAT All-Sky Survey (RASS) X-ray sources. We generated lightcurves for about 30000 X-ray point sources detected sufficiently high above background. For our variability study…

Astrophysics · Physics 2009-11-07 B. Fuhrmeister , J. H. M. M. Schmitt

We investigate the X-ray properties of three interacting luminous infrared galaxy systems. In one of these systems, IRAS 18329+5950, we resolve two separate sources. A second, IRAS 20550+1656, and third, IRAS 19354+4559, have only a single…

We present the results of an homogeneous X-ray analysis for 82 nearby LINERs selected from the catalogue of Carrillo et al. (1999). All sources have available Chandra (68 sources) and/or XMM-Newton (55 sources) observations. This is the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 O. Gonzalez-Martin , J. Masegosa , I. Marquez , M. Guainazzi , E. Jimenez-Bailon

In recent work with high-resolution grating spectrometers (RGS) aboard XMM-Newton Pinto et al. (2016) have discovered that two bright and archetypal ultraluminous X-ray sources (ULXs) have strong relativistic winds in agreement with…

High Energy Astrophysical Phenomena · Physics 2017-05-03 C. Pinto , W. Alston , R. Soria , M. J. Middleton , D. J. Walton , A. D. Sutton , A. C. Fabian , H. Earnshaw , R. Urquhart , E. Kara , T. P. Roberts

We present an analysis of the X-ray emission of a large sample of z~3 Lyman break galaxies (LBGs), based on Chandra/ACIS observations of several LBG survey fields. 24 LBGs are directly detected in the X-ray. 13 of the LBGs have optical…

Astrophysics · Physics 2009-11-11 E. S. Laird , K. Nandra , A. Hobbs , C. C. Steidel

We present a compilation of spectral energy distributions of 35 weak AGNs in LINERs using recent data from the published literature. We make use of previously published compilations of data, after complementing and extending them with more…

Astrophysics of Galaxies · Physics 2015-05-18 Michael Eracleous , Jason A. Hwang , Helene M. L. G. Flohic

We present the results from the high resolution Chandra observation of the Cartwheel galaxy. Many individual sources are resolved in the image, mostly associated with the outer ring. All detected sources have a very high X-ray luminosity…

Astrophysics · Physics 2009-11-10 Anna Wolter , Ginevra Trinchieri

The first high resolution Spitzer IRS 9-37um spectra of 29 Seyfert galaxies (about one quarter) of the 12um Active Galaxy Sample are presented and discussed. The high resolution spectroscopy was obtained with corresponding off-source…

We present an analysis of the extreme obscuration variability observed during an XMM-Newton 5-days continuous monitoring of the AGN in NGC 1365. The source was in a reflection-dominated state in the first ~1.5 days, then a strong increase…

Statistical properties of X-ray luminosity and temperature are studied for 52 early-type galaxies based on the ROSAT PSPC data. All of the X-ray luminous galaxies show largely extended emission with a radius of a few times of 10$r_e$, while…

Astrophysics · Physics 2009-10-31 Kyoko Matsushita

Using the X-ray data taken with ASCA, a detailed analysis was made of intensity and spectral variations of three ultra-luminous extra-galactic compact X-ray sources (ULXs); IC 342 source 1, M81 X-6, and NGC 1313 source B, all exhibiting…

Astrophysics · Physics 2009-11-06 T. Mizuno , A. Kubota , K. Makishima

We present the results of a 17 ks Chandra ACIS-S observation of the nearby dwarf spiral galaxy NGC 4395. Chandra affords the first high-quality, broadband X-ray detection of the active nucleus of this object that is uncontaminated by nearby…

Recent studies of the cosmic X-ray background (XRB) have suggested the possible existence of a population of relatively faint sources with hard X-ray spectra; however, the emission mechanism remains unclear. If the hard X-ray emission is…

Astrophysics · Physics 2007-05-23 Insu Yi , Stephen P. Boughn

We examine the X-ray point source population and 2-10 keV luminosity for two galaxies with high star formation rates (SFRs), NGC 4194 and NGC 7541. The X-ray point source luminosity function (XLF) for these two galaxies is consistent with…

Astrophysics · Physics 2009-11-13 Philip Kaaret , Almudena Alonso-Herrero

We present preliminary results from a XMM-Newton spectroscopic survey of hard (2 -10 keV) X-ray sources detected serendipitously in seven EPIC FOVs. All observations were performed during the performance/verif ication phase. The resulting…

Astrophysics · Physics 2007-05-23 E. Piconcelli , L. Bassani , M. Cappi , F. Fiore , G. Di Cocco , M. Trifoglio

I analyze 101 observations from the ROSAT archive to search for X-ray sources in or near 55 globular clusters. New sources are found in the cores of NGC362 (a double source), NGC6121 (marginally significant), NGC6139, and NGC6266; and…

Astrophysics · Physics 2009-10-31 Frank Verbunt

A growing number of early Be stars discovered in X-ray surveys exhibit X-ray luminosities intermediate between those of normal stars and those of most Be/X-ray binaries in quiescence. Their X-ray spectra are also much harder than those of…

XMM-Newton EPIC observations have revealed a bright point-like X-ray source in the nearby Magellanic-type galaxy NGC 55. At the distance of NGC 55, the maximum observed X-ray luminosity of the source, designated as XMMU J001528.9-391319, is…

Astrophysics · Physics 2009-11-10 A-M. Stobbart , T. P. Roberts , R. S. Warwick

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…

High Energy Astrophysical Phenomena · Physics 2015-06-12 B. Binder , B. F. Williams , M. Eracleous , T. J. Gaetz , A. K. H. Kong , E. D. Skillman , D. R. Weisz

In this paper we investigate the properties of low X-ray-to-optical flux ratio sources detected in a wide area (2.5deg^2) shallow (f(0.5-8keV)~10e-14cgs) XMM-Newton survey. We find a total of 26 sources (5% of the total X-ray selected…