English
Related papers

Related papers: X-ray Bright QSO's around NGC 3079

200 papers

A strong X-ray source only 8" from the nucleus of the Sy2 galaxy NGC 7319 in Stephan's Quintet has been discovered by Chandra. We have identified the optical counterpart and show it is a QSO with $z_e = 2.114$. It is also a ULX with $L_x =…

Astrophysics · Physics 2009-11-10 Pasquale Galianni , E. M. Burbidge , H. Arp , V. Junkkarinen , G. Burbidge , Stefano Zibetti

Two type I X-ray bursts were detected from a position consistent with the transient X-ray source in NGC 6652 with the Wide Field Camera of the BeppoSAX satellite, strongly suggesting that this transient is a neutron star. Our detection…

Galactic X-ray emission is a manifestation of various high-energy phenomena and processes. The brightest X-ray sources are typically accretion-powered objects: active galactic nuclei and low- or high-mass X-ray binaries. Such objects with…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Q. Daniel Wang

An enigmatic, small class of IR and X-ray luminous sources, named ``Composite'' starburst/Seyfert galaxies, has been defined from IRAS and RASS data. The objects have optical spectra dominated by the features of HII galaxies (plus, in some…

The starburst / AGN galaxy M82 was studied by Dahlem, Weaver and Heckman using X-ray data from ROSAT and ASCA, as part of their X-ray survey of edge-on starburst galaxies. They found seventeen unresolved hard-X-ray sources around M82, in…

Astrophysics · Physics 2009-11-07 E. M. Burbidge , G. Burbidge , H. C. Arp , S. Zibetti

We report new Chandra hard X-ray ($>2\rm~keV$) and JVLA C-band observations of the nuclear superbubble of NGC 3079, an analog of the "Fermi bubble" in our Milky Way. We detect extended hard X-ray emission on the SW side of the galactic…

High Energy Astrophysical Phenomena · Physics 2019-03-06 Jiang-Tao Li , Edmund Hodges-Kluck , Yelena Stein , Joel N. Bregman , Judith A. Irwin , Ralf-Jurgen Dettmar

We report preliminary results from an arcsecond-resolution X-ray survey of nearby galaxies using ACIS on board Chandra. The total sample consists of 41 low-luminosity AGNs, including Seyferts, LINERs, and LINER/H II transition objects. In…

The X-ray properties of 15 nearby (v<3,000 km/s) galaxies that possess AGN and/or starbursts are discussed. Two-thirds have nuclear extended emission on scales from ~0.5 to ~1.5 kpc that is either clearly associated with a nuclear outflow…

Astrophysics · Physics 2007-05-23 Kimberly A. Weaver

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…

Astrophysics · Physics 2009-11-10 Roberto Soria , Christian Motch

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

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…

Astrophysics · Physics 2009-11-06 A. J. Young , A. S. Wilson , P. L. Shopbell

Obscured active galactic nuclei, which are classified optically as type 2 (narrow-line) Seyfert galaxies in the local universe, are by far the most promising candidates for the origin of the hard (2-10 keV) X-ray background radiation.…

Astrophysics · Physics 2009-11-07 E. C. Moran , A. V. Filippenko , R. Chornock

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…

The temporal and spectral properties of ultraluminous X-ray sources (ULXs, L>2x10^39 ergs/s) and bright X-ray sources (L>3x10^38 ergs/s) are examined and compared in two extremely different host environments: the old elliptical galaxy NGC…

Astrophysics · Physics 2008-11-26 Hua Feng , Philip Kaaret

The estimate of the number and space density of obscured AGN over cosmic time still represents an open issue. While the obscured AGN population is a key ingredient of the X-ray background synthesis models and is needed to reproduce its…

Astrophysics of Galaxies · Physics 2019-05-29 M. -M. La Caria , C. Vignali , G. Lanzuisi , C. Gruppioni , F. Pozzi

We use the extensive public archive of ROSAT High Resolution Imager (HRI) observations to carry out a statistical investigation of the X-ray properties of nearby galaxies. Specifically we focus on the sample of 486 bright (B_T < 12.5)…

Astrophysics · Physics 2009-10-31 T. P. Roberts , R. S. Warwick

We present an analysis of the X-ray bright point source population in 43 massive clusters of galaxies observed with the Chandra X-ray Observatory. We have constructed a catalog of 4210 rigorously selected X-ray point sources in these…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 S. Ehlert , S. W. Allen , W. N. Brandt , Y. Q. Xue , B. Luo , A. von der Linden , A. Mantz , R. G. Morris

We present an analysis of the compact X-ray source population in the Seyfert~2 galaxy NGC 1068, imaged with Chandra. We find a total of 84 compact sources, of which 66 are projected onto the galactic disk of NGC 1068. Spectra of the…

Astrophysics · Physics 2009-11-07 David A. Smith , Andrew S. Wilson

We present results from the cross-correlation of the spectroscopic atlas of Ho etal (1995) with the ROSAT All-Sky Survey Bright Source Catalogue, in an attempt to understand the X-ray emission mechanisms in nearby galaxies. The resulting…

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

We report on the {\it Chandra} observations of the elliptical galaxy NGC 1399, concentrating on the X-ray sources identified with globular clusters (GCs). A large fraction of the 2-10 keV X-ray emission in the $8' \times 8'$ {\it Chandra}…

Astrophysics · Physics 2019-08-17 Lorella Angelini , Michael Loewenstein , Richard F. Mushotzky