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相关论文: High Resolution X-ray Imaging Observations of two …

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We present an X-ray spectral and spatial analysis of the composite starburst/Seyfert galaxy NGC 1365. Excellent fits of the ROSAT PSPC spectrum are obtained by combining a soft thermal component with a hard powerlaw. The hard component may…

天体物理学 · 物理学 2007-05-23 Stefanie Komossa , Hartmut Schulz

Archival XMM-Newton data on the nearby Seyfert galaxy NGC 4051, taken in relatively high and low flux states, offer a unique opportunity to explore the complexity of its X-ray spectrum. We find the hard X-ray band to be significantly…

天体物理学 · 物理学 2009-11-10 K. A. Pounds , J. N. Reeves , A. R. King , K. L. Page

We present intensive quasi-simultaneous X-ray and radio monitoring of the narrow line Seyfert 1 galaxy NGC 4051, over a 16 month period in 2000-2001. Observations were made with the Rossi Timing X-ray Explorer (RXTE) and the Very Large…

高能天体物理现象 · 物理学 2015-05-20 Sadie Jones , Ian McHardy , Derek Moss , Nick Seymour , Elme Breedt , Phil Uttley , Elmar Kording , Valeriu Tudose

We report results from a Suzaku observation of the narrow-line Seyfert 1 NGC 4051. During our observation, large amplitude rapid variability is seen and the averaged 2--10 keV flux is 8.1x10^-12 erg s^-1 cm^-2, which is several times lower…

We report on the results of a three-year program of coordinated X-ray and optical monitoring of the narrow-line Seyfert 1 galaxy NGC 4051. The rapid continuum variations observed in the X-ray spectra are not detected in the optical,…

NGC 4051 is one of the X-ray brightest and most variable Seyfert galaxies. During 2009 NGC 4051 was caught at its lowest state ever observed by $XMM-Newton$. The low source continuum emission allows a clear measurement of the He-like…

星系天体物理 · 物理学 2019-07-17 Uria Peretz , Jon M. Miller , Ehud Behar

We present a spectral and spatial analysis of the nuclear and circumnuclear X-ray emission of the prominent southern starburst/Seyfert galaxy NGC 1365. To describe the X-ray spectrum of the core source, we favour a two-component model…

天体物理学 · 物理学 2007-05-23 Stefanie Komossa , Hartmut Schulz

New observations using narrow band imaging, long-slit spectroscopy and MERLIN observations of the nuclear region of the Seyfert galaxy NGC~4051 have been made. An edge brightened, triangular region of ionized gas extending 420 pc from the…

Recent radio VLBI observations of the ~parsec-scale nuclear region of the narrow line Seyfert 1 galaxy NGC 4051 hint toward the presence of outflowing plasma. From available literature we have collected high-quality, high-resolution…

高能天体物理现象 · 物理学 2015-05-28 Dipankar Maitra , Jon M. Miller , Sera Markoff , Ashley King

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 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…

天体物理学 · 物理学 2009-11-06 A. J. Young , A. S. Wilson , P. L. Shopbell

We present the first Chandra/ACIS imaging study of the circumnuclear region of the nearby Seyfert galaxy NGC 1365. The X-ray emission is resolved into point-like sources and complex, extended emission. The X-ray morphology of the extended…

星系天体物理 · 物理学 2011-02-11 Junfeng Wang , G. Fabbiano , M. Elvis , G. Risaliti , J. M. Mazzarella , J. H. Howell , S. Lord

We present and analyze a pointed ROSAT PSPC observation of the Seyfert galaxy NGC 4051. The X-ray spectrum consists of a powerlaw modified by absorption edges and an additional soft excess during the high-state in source flux. Modeling the…

天体物理学 · 物理学 2007-05-23 Stefanie Komossa , Henner Fink

Based on our long (~ 300 ks) 2007 XMM-Newton observation of the Seyfert galaxy NGC 1365, we report here on the spectral and timing behaviour of two ultraluminous X-ray sources, which had previously reached isotropic X-ray luminosities L_X ~…

高能天体物理现象 · 物理学 2011-02-11 Roberto Soria , Guido Risaliti , Martin Elvis , Giuseppina Fabbiano , Stefano Bianchi , Zdenka Kuncic

NGC 4051 is a nearby (16.7 Mpc), Narrow Line Seyfert 1 galaxy (NLS1), which has a low black hole mass of $10^6$ M$_{\odot}$. It is also known for its rapid X-ray variability, on timescales of kilo-seconds and has a complex, multi component…

We report on the X-ray spectral variability of the Seyfert 1 galaxy NGC 4051 observed with the Rossi X-ray Timing Explorer (RXTE) during a 1000 day period between May 1996 and March 1999. The spectra were obtained as part of monitoring…

天体物理学 · 物理学 2009-11-07 G. Lamer , I. M. McHardy , P. Uttley , K. Jahoda

We present analysis of the long-term X-ray spectral variability of Seyfert galaxies as observed by Swift, which provides well-sampled observations over a much larger flux range and a much longer timescale than any other X-ray observatory.…

高能天体物理现象 · 物理学 2015-02-27 S. D. Connolly , I. M. McHardy , T. Dwelly

On 9-11 May 1998, the highly-variable, low luminosity Seyfert 1 galaxy NGC4051 was observed in an unusual low flux state by BeppoSAX (Guainazzi et al. 1998) RXTE and EUVE. We present fits of the 4-15 keV RXTE spectrum and BeppoSAX MECS…

天体物理学 · 物理学 2009-10-31 P. Uttley , I. M. McHardy , I. E. Papadakis , M. Guainazzi , A. Fruscione

This paper presents the results of a dense and intensive X-ray and optical monitoring of the narrow-line Seyfert 1 galaxy NGC 4051 carried out in 2000. Results of the optical analysis are consistent with previous measurements. The amplitude…

天体物理学 · 物理学 2009-11-07 O. Shemmer , P. Uttley , H. Netzer , I. M. McHardy

We discuss the origin of the optical variations in the Narrow line Seyfert 1 galaxy NGC 4051 and present the results of a cross-correlation study using X-ray and optical light curves spanning more than 12 years. The emission is highly…

星系天体物理 · 物理学 2015-05-14 E. Breedt , I. M. McHardy , P. Arevalo , P. Uttley , S. G. Sergeev , T. Minezaki , Y. Yoshii , Y. Sakata , P. Lira , N. G. Chesnok
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