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相关论文: NGC 4051: Black hole mass and photon index-mass ac…

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We present the discovery of correlations between the X-ray spectral (photon) index and mass accretion rate observed in active galactic nuclei (AGNs) 3C~454.3 and M87. We analyzed spectral transition episodes observed in these AGNs using…

星系天体物理 · 物理学 2020-01-22 Lev Titarchuk , Elena Seifina , Alexandre Chekhtma , Indira Ocampo

We report the results of Swift and Chandra observations of an ultra-luminous X-ray source, ULX-1 in M101. We show strong observational evidence that M101 ULX-1 undergoes spectral transitions from the low/hard state to the high/soft state…

高能天体物理现象 · 物理学 2015-12-23 Lev Titarchuk , Elena Seifina

We present the results of a reverberation-mapping program targeting NGC5273, a nearby early-type galaxy with a broad-lined active galactic nucleus. Over the course of the monitoring program, NGC5273 showed strong variability that allowed us…

In a recent work we demonstrated that a novel X-ray scaling method, originally introduced for Galactic black holes (GBHs), can be reliably extended to estimate the mass of supermassive black holes accreting at a moderate to high level. Here…

高能天体物理现象 · 物理学 2015-06-19 I. Jang , M. Gliozzi , C. Hughes , L. Titarchuk

We present over 6.5 years of frequent X-ray observations of the NLS1 galaxy NGC4051 by RXTE together with a >100ks observation by XMM-Newton and so derive a 2-10 keV PSD covering an unprecedent frequency range of over 6.5 decades from…

天体物理学 · 物理学 2008-11-26 I. M. McHardy , I. E. Papadakis , P. Uttley , M. J. Page , K. O. Mason

We present a comprehensive examination of the X-ray variability of the narrow line Seyfert 1 (NLS1) galaxy NGC4051. We combine over 6.5 years of frequent monitoring observations by RXTE with a >100ks continuous observation by XMM-Newton and…

天体物理学 · 物理学 2009-11-10 I. M. McHardy , I. E. Papadakis , P. Uttley , K. O. Mason , M. J. Page

The determination of the central black hole mass is crucial to the understanding of AGN physics. In this paper we briefly review some methods that are currently used to estimate the black hole mass of AGNs. Particularly we demonstrate the…

天体物理学 · 物理学 2007-05-23 Xue-Bing Wu , F. K. Liu , R. Wang , M. Z. Kong , J. L. Han

We present a study of correlations between X-ray spectral and timing properties observed from a number of Galactic Black Hole (BH) binaries during hard-soft state spectral evolution. We analyze 17 transition episodes from 8 BH sources…

高能天体物理现象 · 物理学 2011-02-11 Nickolai Shaposhnikov , Lev Titarchuk

We performed a detailed broadband spectral and timing analysis of a small flaring event of ~120 ks in a narrow-line Seyfert 1 galaxy NGC 4051 using simultaneous XMM-Newton and NuSTAR observations. The ~300 ks long NuSTAR observation and the…

高能天体物理现象 · 物理学 2023-03-29 Neeraj Kumari , Arghajit Jana , Sachindra Naik , Prantik Nandi

We report on the results of a simultaneous monitoring campaign employing eight Chandra X-ray (0.5-10 keV) and six VLA/EVLA (8.4 GHz) radio observations of NGC 4051 over seven months. Evidence for compact jets is observed in the 8.4 GHz…

We derive masses of the central super-massive black hole (SMBH) and accretion rates for 154 type1 AGN belonging to a well-defined X-ray-selected sample, the XMM-Newton Serendipitous Sample (XBS). To this end, we use the most recent…

宇宙学与河外天体物理 · 物理学 2015-06-12 A. Caccianiga , R. Fanali , P. Severgnini , R. Della Ceca , E. Marchese , S. Mateos

NGC 6240 is a pair of colliding disk galaxies, each with a black hole in its core. We have used laser guide star adaptive optics on the Keck II telescope to obtain high-resolution ($\sim 0.06$") near-infrared integral-field spectra of the…

宇宙学与河外天体物理 · 物理学 2015-05-30 Anne M. Medling , S. Mark Ammons , Claire E. Max , Richard I. Davies , Hauke Engel , Gabriela Canalizo

We present an analysis of the fundamental plane of black hole accretion, an empirical correlation of the mass of a black hole ($M$), its 5 GHz radio continuum luminosity ($\nu L_{\nu}$), and its 2-10 keV X-ray power-law continuum luminosity…

We present an XMM-Newton time-resolved spectral analysis of the NLS1 galaxy Mrk 766. We analyse eight available observations of the EPIC-pn camera taken between May 2000 and June 2005 to investigate the X-ray spectral variability as…

高能天体物理现象 · 物理学 2015-06-17 S. Giacche` , R. Gilli , L. Titarchuk

We present a revised measurement of the mass of the central black hole (Mbh) in the Seyfert 1 galaxy NGC 4151. The new stellar dynamical mass measurement is derived by applying an axisymmetric orbit-superposition code to near-infrared…

We present a study of the correlations between spectral, timing properties and mass accretion rate observed in X-rays from the Galactic Black Hole (BH) binary GRS 1915+105 during the transition between hard and soft states. We analyze all…

高能天体物理现象 · 物理学 2014-11-20 Lev Titarchuk , Elena Seifina

Accurately determining the black hole mass ($M_\mathrm{BH}$) in active galactic nuclei (AGN) is crucial to constraining their properties and to studying their evolution. While direct methods yield reliable measurements of $M_\mathrm{BH}$ in…

星系天体物理 · 物理学 2023-03-29 James K. Williams , Mario Gliozzi , Kyle A. Bockwoldt , Onic I. Shuvo

We present our analysis of X-ray spectral properties observed from the Seyfrert 1 galactic nucleus NGC~7469 using the RXTE and ASCA observations. We demonstrate strong observational evidence that NGC~7469 undergoes spectral transitions from…

星系天体物理 · 物理学 2018-11-14 Elena Seifina , Lev Titarchuk , Lyubov Ugolkova

We model the spectral energy distribution of the type 1 Seyfert galaxy NGC 5548, fitting data from simultaneous optical, UV, and X-ray monitoring observations. We assume a geometry consisting of a hot central Comptonizing region surrounded…

天体物理学 · 物理学 2009-11-07 James Chiang , Omer Blaes

Using bonafide black hole (BH) mass estimates from reverberation mapping and the line ratio [Si VI]1.963$\mu$m/Br$\gamma_{\rm broad}$ as tracer of the Active Galactic Nuclei (AGN) ionizing continuum, we find a novel BH-mass scaling relation…

星系天体物理 · 物理学 2021-11-30 Swayamtrupta Panda , Alberto Rodríguez Ardila
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