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We study the prototypical Seyfert 2 galaxy, Markarian 3, based on imaging and high-resolution spectroscopy observations taken by the Chandra X-ray Observatory. We construct a deconvolved X-ray image, which reveals the S-shaped morphology of…

高能天体物理现象 · 物理学 2017-10-18 Akos Bogdan , Ralph P. Kraft , Daniel A. Evans , Felipe Andrade-Santos , William R. Forman

NGC 1365 is a Seyfert 2 galaxy with a starburst ring in its nuclear region. In this work we look at the XMM Reflection Grating Spectrometer (RGS) data from four 2012-13, three 2007 and two 2004 observations of NGC 1365. We characterise the…

高能天体物理现象 · 物理学 2016-11-03 M. Whewell , G. Branduardi-Raymont , M. J. Page

We present a sample of 8 nearby Seyfert 2 galaxies observed by HST and Chandra. All of the sources present soft X-ray emission which is coincident in extension and overall morphology with the [OIII] emission. The spectral analysis reveals…

天体物理学 · 物理学 2009-11-11 Stefano Bianchi , Matteo Guainazzi , Marco Chiaberge

We present spatially resolved Chandra HETGS observations of the Seyfert 2 galaxy NGC 1068. X-ray imaging and high resolution spectroscopy are used to test the Seyfert unification theory. Fe K-alpha emission is concentrated in the nuclear…

天体物理学 · 物理学 2009-11-07 P. M. Ogle , T. Brookings , C. R. Canizares , J. C. Lee , H. L. Marshall

We report BeppoSAX observations of spatially resolved hard X-ray emission from IC 443, a supernova remnant interacting with a molecular cloud. The emission is shown to come from two localized features spatially correlated with bright…

天体物理学 · 物理学 2007-05-23 F. Bocchino , A. M. Bykov

The inner-most region of the Seyfert galaxy NGC 2992 has long been suspected to be the location of intense AGN-host galaxy interaction, but photon pile-up in previous high-resolution observations hampered the study of soft X-ray excess and…

星系天体物理 · 物理学 2022-10-26 Xiaoyu Xu , Junfeng Wang

We present Chandra observations of the X-ray environment of a sample of 6 BL Lacertae objects. The improved sensitivity of the ACIS experiment allows us to separate the core X-ray emission from the contribution of diffuse emission from the…

天体物理学 · 物理学 2009-11-07 D. Donato , M. Gliozzi , R. M. Sambruna , J. E. Pesce

We present the Chandra analysis of the galaxy cluster A521 (z=0.247). The high resolution of the Chandra observation has allowed us to refine the original merging scenario proposed for A521, and to reveal new features in its X-ray emission.…

天体物理学 · 物理学 2009-11-11 C. Ferrari , M. Arnaud , S. Ettori , S. Maurogordato , J. Rho

We analyze Chandra observations of diffuse soft X-ray emission associated with a complete sample of 3CR radio galaxies at z < 0.3. In this paper we focus on the properties of the spectroscopic sub-classes of high excitation galaxies (HEGs)…

Sub-arcsecond resolution Chandra observations of Eta Carinae reveal a 40 arcsec X 70 arcsec ring or partial shell of X-ray emission surrounding an unresolved, bright, central source. The spectrum of the central source is strongly absorbed…

天体物理学 · 物理学 2009-11-06 F. D. Seward , Y. M. Butt , M. Karovska , A. Prestwich. E. M. Schlegel , M. Corcoran

The nature of the extended hard X-ray source XMMU J061804.3+222732 and its surroundings is investigated using XMM-Newton, Chandra, and Spitzer observations. This source is located in an interaction region of the IC 443 supernova remnant…

In this letter we report the detection of an extremely strong X-ray emission line in the 940ks chandra ACIS-I spectrum of CXO CDFS J033225.3-274219. The source was identified as a Type1 AGN at redshift of z = 1.617, with 2.0 -- 10.0 keV…

天体物理学 · 物理学 2015-06-24 J. Wang , T. Yaqoob , G. Szokoly , R. Gilli , L. Kewley , V. Mainieri , M. Nonino , P. Rosati , P. Tozzi , W. Zheng , A. Zirm , C. Norman

We report Chandra ACIS and quasi-simultaneous RXTE observations of the nearby, powerful radio galaxy Cygnus A, with the present paper focusing on the properties of the active nucleus. In the Chandra observation, the hard (> a few keV) X-ray…

天体物理学 · 物理学 2009-11-07 Andrew J. Young , Andrew S. Wilson , Yuichi Terashima , Keith A. Arnaud , David A. Smith

We investigate the origin of the soft X-ray excess emission from narrow-line Seyfert 1 galaxies Akn564 and Mrk1044 using XMM-Newton observations. We find clear evidence for time delays between the soft and hard X-ray emission from Akn564…

天体物理学 · 物理学 2009-11-13 G. C. Dewangan , R. E. Griffiths , Surajit Dasgupta , A. R. Rao

We present the first results from 60ks of observations of Arp 220 using the ACIS-S instrument on Chandra. We report the detection of several sources near the galaxy's nucleus, including a point source with a hard spectrum that is coincident…

天体物理学 · 物理学 2009-11-07 D. L. Clements , J. C. McDowell , S. Shaked , A. C. Baker , K. Borne , L. Colina , S. Lamb , C. Mundell

A short Chandra ACIS-S observation of the Seyfert 2 galaxy IC 2560, which hosts a luminous nuclear water megamaser, shows: 1) the X-ray emission is extended; 2) the X-ray spectrum shows emission features in the soft (E<2 keV) X-ray band;…

天体物理学 · 物理学 2009-11-07 K. Iwasawa , P. R. Maloney , A. C. Fabian

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…

We employ MUSE/VLT data to study the ionised and highly ionised gas phases of the feedback in Circinus, the closest Seyfert 2 galaxy to us. The analysis of the nebular emission allowed us to detect a remarkable high-ionisation gas outflow…

星系天体物理 · 物理学 2021-06-28 M. A. Fonseca-Faria , A. Rodríguez-Ardila , M. Contini , V. Reynaldi

We report the detection at X-rays of the radio/optical jet of 3C 371, from a short (10 ks) Chandra exposure in March 2000. We also present a new MERLIN observation at 1.4 GHz together with a renalysis of the archival HST WFPC2 F555W image.…

天体物理学 · 物理学 2009-11-06 Joseph E. Pesce , Rita M. Sambruna , F. Tavecchio , L. Maraschi , C. C. Cheung , C. Megan Urry , R. Scarpa

To investigate the role of active galactic nucleus (AGN) X-ray irradiation on the interstellar medium (ISM), we systematically analyzed Chandra and ALMA CO($J$=2-1) data for 26 ultra-hard X-ray ($>$ 10 keV) selected AGNs at redshifts below…