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相关论文: A Photoionization Model For The Soft X-Ray Spectru…

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We present the Chandra discovery of soft diffuse X-ray emission in NGC 4151 (L[0.5-2keV]~10^{39} erg s$^{-1}$), extending ~2 kpc from the active nucleus and filling in the cavity of the HI material. The best fit to the X-ray spectrum…

Narrow Line Seyfert 1 (NLSy1) galaxies have recently received a lot of attention due to their unusual optical--X-ray properties which are not yet well understood. Photoionization models of the circum-nuclear emission/absorption regions…

天体物理学 · 物理学 2017-07-12 Stefanie Komossa , Janek Meerschweinchen

We present results from Chandra HETGS (250 ks over two epochs) and XMM-Newton EPIC and RGS (60 ks) observations of NGC 2110, which has been historically classified as a Narrow Emission Line Galaxy galaxy. Our results support the…

天体物理学 · 物理学 2009-11-13 Daniel A. Evans , Julia C. Lee , T. Jane Turner , Kimberly A. Weaver , Herman L. Marshall

We present new results from a Chandra HETG observation of NGC 5548 and give a comparison of absorption and emission features found in other Seyfert 1 galaxies using Chandra grating observations. Deep soft X-ray edges are seen in Mkn 509 and…

天体物理学 · 物理学 2007-05-23 T. Yaqoob , I. M. George , T. J. Turner

An extended component of X-ray emission has been detected in Seyfert galaxies - NGC 1365 and NGC 4051, using the ROSAT HRI. Its size is about 2 kpc and it contains 56% +- 8% of the total observed flux in NGC 1365, and 21% +- 6% in NGC 4051.…

天体物理学 · 物理学 2009-09-25 Kulinder Pal Singh

We present modeling and interpretation of the continuum and emission lines for a sample of 51 unobscured Type 1 active galactic nuclei (AGN). All of these AGNs have high quality spectra from both XMM-Newton and Sloan Digital Sky Survey…

高能天体物理现象 · 物理学 2015-05-30 C. Jin , M. Ward , C. Done , J. M. Gelbord

We report the results obtained by a broad-band (0.5-500 keV) data analysis of narrow-line Seyfert 1 galaxy NGC 4748 observed with an XMM-Newton/PN, INTEGRAL/ISGRI and SWIFT/BAT telescopes. This galaxy has a soft X-ray excess that is typical…

高能天体物理现象 · 物理学 2018-10-17 Anatoliy Vasylenko

We present high-resolution soft-X-ray spectra of the prototypical Seyfert 2 galaxy, NGC 1068, taken with XMM-Newton RGS and Chandra LETGS. Its rich emission-line spectrum is dominated by recombination in a warm plasma (bright, narrow…

The photoionization models for the narrow emission line regions of powerful radio galaxies have yet to be tested in depth. To this end, we present high-quality long-slit spectroscopy of the powerful double-nucleus radio galaxy 3C 321. The…

天体物理学 · 物理学 2009-10-31 T. G. Robinson , C. N. Tadhunter , D. J. Axon , A. Robinson

We present first INTEGRAL and XMM-Newton observations of a Seyfert galaxy, the type 2 AGN NGC 4388. Several INTEGRAL observations performed in 2003 allow us to study the spectrum in the 20 - 300 keV range. In addition two XMM-Newton…

天体物理学 · 物理学 2009-11-10 V. Beckmann , N. Gehrels , P. Favre , R. Walter , T. J. -L. Courvoisier , P. -O. Petrucci , J. Malzac

The Narrow Line Seyfert 1 galaxy NGC4051 shows unusual low flux states, lasting several months, when the 2-10 keV X-ray spectrum becomes unusually hard (photon index<1) while the spectrum at lower X-ray energies is dominated by a large soft…

天体物理学 · 物理学 2009-11-10 P. Uttley , R. D. Taylor , I. M. McHardy , M. J. Page , K. O. Mason , G. Lamer , A. Fruscione

We observed the Seyfert 1 galaxy Mrk 509 simultaneously with Chandra/HETG, HST/STIS and RXTE. We measure strong absorption lines from He-like Ne and Mg, and from H-like N, O, and Ne. The lines are unresolved except for Ne Lya and Ne IX(r).…

天体物理学 · 物理学 2009-11-07 T. Yaqoob , B. McKernan , S. B. Kraemer , M. Crenshaw , J. Gable , I. M. George , T. J. Turner

We have obtained a broad-band spectrum of the Compton-thick Seyfert 2 galaxy NGC 2273 with Suzaku. The spectrum reveals the first detection of hard X-rays above ~10 keV from NGC 2273. The broad-band spectrum is well represented by a…

天体物理学 · 物理学 2008-10-28 H. Awaki , Y. Terashima , Y. Higaki , Y. Fukazawa

We present results from a 150 ksec Suzaku observation of the Seyfert 1.5 NGC 3516 in October 2005. The source was in a relatively highly absorbed state. Our best-fit model is consistent with the presence of a low-ionization absorber which…

We present recent results from spectroscopic data and modeling of the biconical ionized gas in the Seyfert-2 galaxy NGC 4388. A field of ~2.6 x 2.4 kpc centered on the nucleus has been observed by means of the modern technique of integral…

天体物理学 · 物理学 2009-11-07 S. Ciroi , M. Contini , P. Rafanelli , G. M. Richter

It is widely believed that the primary X-ray emission of AGN is due to the Comptonisation of optical-UV photons from a hot electron corona, while the origin of the 'soft-excess' is still uncertain and matter of debate. A second…

高能天体物理现象 · 物理学 2018-12-19 R. Middei , S. Bianchi , P. -O. Petrucci , F. Ursini , M. Cappi , B. De Marco , A. De Rosa , J. Malzac , A. Marinucci , G. Matt , G. Ponti , A. Tortosa

A series of {\sl ROSAT\/}, {\sl ASCA\/} and Compton Gamma-Ray Observatory ({\sl CGRO\/}) observations of the Seyfert galaxy NGC 4151 were carried out during the period 1993 November 30 to December 13 as part of an intensive campaign to…

天体物理学 · 物理学 2009-10-28 R. S. Warwick et al

We present a spectral and imaging analysis of the XMM-Newton and Chandra observations of the Seyfert 2 galaxy ESO138-G001, with the aim of characterizing the circumnuclear material responsible for the soft (0.3-2.0 keV) and hard (5-10 keV)…

星系天体物理 · 物理学 2015-09-09 M. De Cicco , A. Marinucci , S. Bianchi , E. Piconcelli , G. Violino , C. Vignali , F. Nicastro

We present the results from simultaneous observations of the Narrow-Line Seyfert 1 galaxy NGC 4051 with the Chandra High Energy Transmission Grating Spectrometer and the HST Space Telescope Imaging Spectrograph. The X-ray grating spectrum…

We present high-sensitivity eMERLIN radio images of the Seyfert galaxy NGC 4151 at 1.5 GHz. We compare the new eMERLIN images to those from archival MERLIN observations in 1993 to determine the change in jet morphology in the 22 years…