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Related papers: Soft X-ray Emission from the Spiral Galaxy NGC 131…

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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 describe a series of observations of NGC 1313 using the ROSAT HRI with a combined exposure time of 183.5 ksec. The observations span an interval between 1992 and 1998; the purpose of observations since 1994 was to monitor the X-ray flux…

Astrophysics · Physics 2009-10-31 Eric M. Schlegel , Robert Petre , E. J. M. Colbert , Scott Miller

The emission-line dwarf galaxy NGC 3413 is known to host a bright X-ray source near its optical center. The 0.3-10 keV luminosity of this source is estimated to be approximately 10$^{39}$ erg$s^{-1}$ potentially qualifying it as an…

High Energy Astrophysical Phenomena · Physics 2018-10-17 E. Sonbas , K. S. Dhuga , E. Göğüş

We present new optical and {\it Chandra} observations of the field containing the ultraluminous X-ray source NGC 1313 X-2. On an ESO 3.6 m image, the {\it Chandra} error box embraces a $R=21.6$ point-like object and excludes a previously…

We present an XMM-Newton observation of the massive edge-on Sb galaxy NGC 2613. We discover that this galaxy contains a deeply embedded active nucleus with a 0.3-10 keV luminosity of 3.3x10^40 erg/s and a line-of-sight absorption column of…

Astrophysics · Physics 2009-11-11 Zhiyuan Li , Q. Daniel Wang , Judith A. Irwin , Tara Chaves

We present a spectral and spatial analysis of the nuclear and circumnuclear X-ray emission of the prominent southern starburst/Seyfert galaxy NGC 1365. To describe the X-ray spectrum of the core source, we favour a two-component model…

Astrophysics · Physics 2007-05-23 Stefanie Komossa , Hartmut Schulz

The nearby barred spiral galaxy NGC 1672 is thought to have a weak Seyfert nucleus in addition to its strong starburst activity. Observations with the PSPC and HRI instruments on board the ROSAT X-ray satellite show that three X-ray sources…

Astrophysics · Physics 2015-06-24 W. N. Brandt , J. P. Halpern , K. Iwasawa

Chandra has resolved the starburst nuclear region of the face-on grand-design spiral M83. Eighty-one point sources are detected above 3.5 sigma in the ACIS S3 image, and 15 of them are within the inner 16-arcsec region of the galaxy. A…

Astrophysics · Physics 2009-11-07 Roberto Soria , Kinwah Wu

The E3 giant elliptical galaxy NGC5018 was observed with the Chandra X-ray Observatory on 14 April 2001. Results of analysis of these X-ray data as well as of complementary optical, infrared, and radio data are reported. Seven X-ray point…

Astrophysics · Physics 2009-11-10 Kajal K. Ghosh , Douglas A. Swartz , Allyn F. Tennant , Kinwah Wu , Lakshmi Saripalli

The nearby barred spiral galaxy NGC 1672 shows dramatic starburst activity and may also host a Seyfert 2 nucleus. We present new X-ray observations that set constraints on starburst and Seyfert activity in NGC 1672. Two ROSAT HRI exposures,…

Astrophysics · Physics 2009-10-31 P. J. de Naray , W. N. Brandt , J. P. Halpern , K. Iwasawa

We report the results of a deep spatial, spectral, and timing analysis of ROSAT HRI and PSPC observations of the edge-on starburst galaxy NGC 253. In this first paper, point-like X-ray sources detected within the galaxy and in the field are…

Astrophysics · Physics 2007-05-23 A. Vogler , W. Pietsch

We present evidence of the co-existence of either an AGN or an ultraluminous X-ray source (ULX), together with a young super stellar cluster in the 3 central parsecs of NGC4303. The galaxy contains a low luminosity AGN and hosts a number of…

(Abridged) We present a deep Chandra observation of the late-type barred spiral galaxy NGC 2903. The Chandra data reveal soft (kT_e ~ 0.2-0.5keV) diffuse emission in the nuclear starburst region and extending ~5kpc to the north and west of…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 Mihoko Yukita , Douglas A. Swartz , Allyn F. Tennant , Roberto Soria , Jimmy A. Irwin

NGC 1313 is a bulgeless nearby galaxy, classified as SB(s)d. Its proximity allows high spatial resolution observations. We performed the first detailed analysis of the emission-line properties in the nuclear region of NGC 1313, using an…

Astrophysics of Galaxies · Physics 2017-01-20 R. B. Menezes , J. E. Steiner

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…

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

Recent Chandra ACIS-S observations have detected a point source at the central star of NGC 6543 and confirmed the point source nature of the hard X-ray emission from NGC 7293. The X-ray spectra of both sources peak between 0.5 keV and 1.0…

We report the results of XMM-Newton observations for an especially luminous supersoft X-ray source (SSS) with bolometric luminosity of 10^39 erg/s in the spiral galaxy NGC 300. The source was detected as a SSS in 1992 and disappeared in…

Astrophysics · Physics 2009-11-07 A. K. H. Kong , R. Di Stefano

We report here the results of a full analysis of all the ROSAT PSPC spectral imaging observations and all the ROSAT HRI high resolution imaging observations of the very nearby (D=2.1 Mpc) Sculptor galaxy, NGC 300. Many point sources are…

Astrophysics · Physics 2009-11-06 A. M. Read , W. Pietsch

Two ultraluminous X-ray sources (ULXs) in the nearby Sb galaxy NGC 1313, named X-1 and X-2, were observed with Suzaku on 2005 September 15. During the observation for a net exposure of 28~ks (but over a gross time span of 90~ks), both…

In this paper, we report a detailed study with a variety of data from optical, near-infrared, X-ray, and radio telescopes of the nuclear region of the galaxy NGC 613 with the aim of understanding its complexity. We detected an extended…

Astrophysics of Galaxies · Physics 2020-01-22 Patrícia da Silva , Roberto B. Menezes , João E. Steiner
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