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相关论文: NGC 5252 - a Liner undercover

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XMM-Newton and Chandra/HETG spectra of the Compton-thin (NH 4x10^{23} cm^{-2}) Seyfert 2 galaxy, NGC 4507, are analyzed and discussed. The main results are: a) the soft X-ray emission is rich in emission lines; an (at least) two--zone…

天体物理学 · 物理学 2009-11-10 Giorgio Matt , Stefano Bianchi , Filippo D'Ammando , Andrea Martocchia

A deep 75 ks {\it Chandra} ACIS--I data of NGC 2024 was analyzed, aiming at a search for diffuse X-ray emission in this one of the most nearby (415 pc) massive star-forming regions. After removing point sources, an extended emission was…

天体物理学 · 物理学 2009-11-11 Yuichiro Ezoe , Motohide Kokubun , Kazuo Makishima , Yutaro Sekimoto , Keiichi Matsuzaki

ASCA observations of the Seyfert 2 galaxy NGC 7582 revealed it was highly variable on the timescale of $\sim2\times10^4$ s in the hard X-ray (2-10 keV) band, while the soft X-ray (0.5-2 keV) flux remained constant during the observations.…

天体物理学 · 物理学 2015-06-24 S. -J. Xue , C. Otani , T. Mihara , M. Cappi , M. Matsuoka

We present T-ReCS high spatial resolution N-band (8-13 micron) spectroscopy of the central regions (a few kpc) of 3 local LIRGs. The nuclear spectra show deep 9.7 micron silicate absorption feature and the high ionization [SIV]10.5 micron…

天体物理学 · 物理学 2007-05-23 T. Diaz-Santos , A. Alonso-Herrero , L. Colina , C. Packham , J. T. Radomski , C. M. Telesco

We report on sensitive dual-frequency (1.7 and 5 GHz) European VLBI Network observations of the central region of nine Seyfert galaxies. These sources are among the faintest and least luminous members of a complete sample of nearby (d<22…

宇宙学与河外天体物理 · 物理学 2015-06-11 P. Bontempi , M. Giroletti , F. Panessa , M. Orienti , A. Doi

All the observations available in the Chandra and XMM-Newton archives have been used to investigate the X-ray spectral properties of 3C 33. In this paper is presented a complete X-ray analysis of the nuclear emission of this narrow line…

高能天体物理现象 · 物理学 2009-11-13 E. Torresi , P. Grandi , M. Guainazzi , G. G. C. Palumbo , G. Ponti , S. Bianchi

The atomic spectra and structure of the open d- and f-shell elements are extremely complex, where tens of thousands of transitions between fine structure energy levels can be observed as spectral lines across the infrared and UV per…

原子物理 · 物理学 2025-01-23 M. Ding , S. Z. J. Lim , X. Yu , C. P. Clear , J. C. Pickering

We study the narrow-line region (NLR) of the Seyfert-2 galaxy NGC 1386 by means of long-slit spectroscopy obtained with FORS1 at the VLT. We use the galaxy itself for subtracting the stellar template, applying reddening corrections to fit…

天体物理学 · 物理学 2009-11-11 Nicola Bennert , Bruno Jungwiert , Stefanie Komossa , Martin Haas , Rolf Chini

We present a study of the outflowing ionized gas in the resolved narrow-line region (NLR) of the Seyfert 2 galaxy Mrk 573, and its interaction with an in- ner dust/gas disk, based on Hubble Space Telescope (HST) WFPC2 and STIS observations.…

宇宙学与河外天体物理 · 物理学 2015-05-19 T. C. Fischer , D. M. Crenshaw , S. B. Kraemer , H. R. Schmitt , M. L. Trippe

We present a study of the global properties of Joguet's sample of 65 Seyfert 2 galaxies. We use the population synthesis models of our Paper II to derive `pure' emission-line spectra, and thus explore the statistical properties of the…

Aims: Our aim is to identify the dominant molecular cooling lines and characteristic emission features in the 1.3 mm window of distinct regions in the northern part of the Orion A molecular cloud. By defining and analysing template regions,…

星系天体物理 · 物理学 2020-04-15 N. Brinkmann , F. Wyrowski , J. Kauffmann , D. Colombo , K. M. Menten , X. D. Tang , R. Güsten

There is now convincing evidence that the intensity of HCN molecular line emission is enhanced around active galactic nuclei. In this paper we examine the specific case of the Seyfert galaxy NGC3227, for which there are subarcsecond…

宇宙学与河外天体物理 · 物理学 2015-06-03 R. Davies , D. Mark , A. Sternberg

We present integral field spectroscopy of NGC 5033, a low luminosity Seyfert galaxy. The observations were made with INTEGRAL, a fiber based system operating at the WHT. The intensity map of the H$\beta$ emission line represents a spiral or…

Extended nebular filaments are seen at optical wavelengths in NGC 1275, the central galaxy in the Perseus cluster. The agents responsible for the excitation of these filaments remain poorly understood. In this paper we investigate possible…

天体物理学 · 物理学 2009-10-31 B. M. Sabra , J. C. Shields , A. V. Filippenko

We study the absorption and emission properties of the photoionised gas near one of the brightest and most variable AGN, the Seyfert galaxy NGC 4051, in order to constrain the geometry, dynamics and ionisation structure of the outflow. We…

天体物理学 · 物理学 2007-05-23 M. Fenovcik , J. S. Kaastra , E. Costantini , K. C. Steenbrugge , F. Verbunt

ABRIDGED: A detailed 2D study of the central region of NGC5253 has been performed to characterize the stellar and ionized gas structure as well as the extinction distribution, physical properties and kinematics of the ionized gas in the…

宇宙学与河外天体物理 · 物理学 2015-05-18 A. Monreal-Ibero , J. M. Vilchez , J. R. Walsh , C. Munoz-Tunon

We present results from a program of optical spectroscopy for 23 nearby galaxy emission-line nuclei. This investigation takes advantage of the spatial resolution of the Hubble Space Telescope to study the structure and energetics of the…

We report the results of a spectropolarimetric survey of a complete far infrared selected sample of Seyfert 2 galaxies. We have found polarized broad Halpha emission in one new source, NGC5995. In the sample as a whole, there is a clear…

天体物理学 · 物理学 2009-11-06 S. L. Lumsden , C. A. Heisler , J. A. Bailey , J. H. Hough , S. Young

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…

We present an analysis of the 101 ks, 2007 Suzaku spectrum of the LINER galaxy NGC 1052. The 0.5-10 keV continuum is well-modeled by a power-law modified by Galactic and intrinsic absorption, and it exhibits a soft, thermal emission…

高能天体物理现象 · 物理学 2011-02-11 L. W. Brenneman , K. A. Weaver , M. Kadler , J. Tueller , A. Marscher , E. Ros , A. Zensus , Y. Y. Kovalev , M. Aller , H. Aller , J. Irwin , J. Kerp , S. Kaufmann