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相关论文: Deep Chandra Observation of the Remarkable Ionizat…

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We present the results of a Chandra soft X-ray observation of the spectacular ionization cone in the nearby Seyfert 2 galaxy NGC 5252. As almost invariably observed in obscured AGN, the soft X-ray emission exhibits a remarkable…

天体物理学 · 物理学 2007-10-09 Matteo Guainazzi , Stefano Bianchi , Massimo Cappi , Mauro Dadina , Giuseppe Malaguti

The physical conditions of the gas forming the narrow line regions (NLR) in active galactic nuclei (AGN) have been extensively studied in the optical band. We take advantage of the spectacular extension ($\sim$15") of the NLR in the type II…

星系天体物理 · 物理学 2015-05-18 M. Dadina , M. Guainazzi , M. Cappi , S. Bianchi , C. Vignali , G. Malaguti , A. Comastri

We present results from HST/STIS long-slit spectroscopy of the gas motions in the nuclear region of the Seyfert 2 galaxy NGC 5252. The observed velocity field is consistent with gas in regular rotation with superposed localized patches of…

天体物理学 · 物理学 2009-11-10 Alessandro Capetti , Alessandro Marconi , Duccio Macchetto , David Axon

Ground based long slit spectroscopic observations of the nuclear region of NGC 5252, and Hubble Space Telescope (HST) Faint Object Spectrograph (FOS) spectra of the nucleus and two bright knots located 0.36" NE and 0.31" SW from it, show…

天体物理学 · 物理学 2007-05-23 A. C. Goncalves , P. Veron , M. -P. Veron-Cetty

Recent observations of nearby Compton thick (CT) active galactic nuclei (AGNs) with Chandra have resolved hard (>3 keV) X-ray emission extending out from the central supermassive black hole to kiloparsec scales, challenging the long-held…

星系天体物理 · 物理学 2020-03-25 Mackenzie L. Jones , G. Fabbiano , Martin Elvis , A. Paggi , M. Karovska , W. P. Maksym , A. Siemiginowska , J. Raymond

We present a detailed imaging analysis of 260 ks of sub-arcsecond resolution Chandra Advanced CCD Imaging Spectrometer (ACIS-S) observations of the nearby Seyfert 2 galaxy NGC 5728. Our study focuses on the bright and diffuse soft X-ray…

星系天体物理 · 物理学 2024-11-01 Anna Trindade Falcao , G. Fabbiano , M. Elvis , A. Paggi , W. P. Maksym

We report the discovery of a ultraluminous X-ray source (ULX; CXO J133815.6+043255) in NGC 5252. This ULX is an off-nuclear point-source, which is 22$^{\prime\prime}$ away from the center of NGC 5252, and has an X-ray luminosity of 1.5…

We present results on Mrk 573 obtained as part of the CHandra survey of Extended Emission-line Regions in nearby Seyfert galaxies (CHEERS). Previous studies showed that this source features a biconical emission in the soft X-ray band…

高能天体物理现象 · 物理学 2015-06-04 Alessandro Paggi , Junfeng Wang , Giuseppina Fabbiano , Martin Elvis , Margarita Karovska

The Seyfert 2 galaxy NGC 5252 contains a recently identified ultra-luminous X-ray (ULX) source that has been suggested to be a possible candidate off-nuclear low-mass active galactic nucleus. We present follow-up optical integral-field unit…

星系天体物理 · 物理学 2017-08-02 Minjin Kim , Luis C. Ho , Myungshin Im

Recent deep Chandra observations of nearby Compton thick (CT) AGN have produced surprising results, uncovering extended emission not only in the soft X-rays but in the hard emission (>3 keV), challenging the long-held belief that the…

星系天体物理 · 物理学 2023-06-28 Anna Trindade Falcao , G. Fabbiano , M. Elvis , A. Paggi , W. P. Maksym

This paper is the third in a series in which we present deep Chandra ACIS-S imaging spectroscopy of the Seyfert 1 galaxy NGC 4151, devoted to study its complex circum-nuclear X-ray emission. Emission features in the soft X-ray spectrum of…

We explore the gas morphology and excitation mechanisms of the ionization cones of the Type II Seyfert galaxy NGC 5728. Near-IR and optical data from the SINFONI and MUSE IFUs on the VLT are combined with $HST$ optical images, $Chandra$…

星系天体物理 · 物理学 2018-11-28 Mark Durré , Jeremy Mould

We present the spatial analysis of five Compton thick (CT) active galactic nuclei (AGNs), including MKN 573, NGC 1386, NGC 3393, NGC 5643, and NGC 7212, for which high resolution Chandra observations are available. For each source, we find…

星系天体物理 · 物理学 2021-03-31 Mackenzie L Jones , K. Parker , G. Fabbiano , M. Elvis , W. P. Maksym , A. Paggi , J. Ma , M. Karovska , A. Siemiginowska , J. Wang

There are few observational constraints on how the escape of ionizing photons from starburst galaxies depends on galactic parameters. Here, we report on the first major detection of an ionization cone in NGC 5253, a nearby starburst galaxy.…

宇宙学与河外天体物理 · 物理学 2015-05-30 Jordan Zastrow , M. S. Oey , Sylvain Veilleux , Michael McDonald , Crystal L. Martin

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…

星系天体物理 · 物理学 2020-01-22 Patrícia da Silva , Roberto B. Menezes , João E. Steiner

We present new optical GTC/MEGARA seeing-limited (0.9") integral-field observations of NGC 5506, together with ALMA observations of the CO(3-2) transition at a 0.2" (25 pc) resolution. NGC 5506 is a luminous (bolometric luminosity of $\sim…

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

Observations of the Seyfert 2 and starburst galaxy NGC 5135 with the Chandra X-ray Observatory demonstrate that both of these phenomena contribute significantly to its X-ray emission. We spatially isolate the active galactic nucleus (AGN)…

天体物理学 · 物理学 2016-08-30 N. A. Levenson , K. A. Weaver , T. M. Heckman , H. Awaki , Y. Terashima

We present the analysis of an optical data cube of the central region of NGC 1448, obtained with the Multi Unit Spectroscopic Explorer (MUSE). Chandra X-ray data indicate that the active galactic nucleus (AGN) is not located at the apparent…

星系天体物理 · 物理学 2021-03-29 R. B. Menezes , Patrícia da Silva , J. E. Steiner

We present the results of the spatial and spectral analysis of the deep (~200 ksec) Chandra HETG observation of the changing look AGN NGC7582. During this observation NGC7582 was in a highly obscured state. Therefore, we considered also a…

高能天体物理现象 · 物理学 2017-04-19 Valentina Braito , James Reeves , Stefano Bianchi , Emanuele Nardini , Enrico Piconcelli
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