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相关论文: Discovery of Polarization Reverberation in NGC 415…

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NGC 4151 is among the most well-studied Seyfert galaxies that does not suffer from strong obscuration along the observer's line-of-sight. This allows to probe the central active galactic nucleus (AGN) engine with photometry, spectroscopy,…

星系天体物理 · 物理学 2020-06-10 F. Marin , J. Le Cam , E. Lopez-Rodriguez , M. Kolehmainen , B. L. Babler , M. R. Meade

Obscuring circumnuclear dust is a well-established constituent of active galactic nuclei (AGN). Traditionally referred to as the receding dusty torus, its inner radius and angular extension should depend on the photo-ionizing luminosity of…

高能天体物理现象 · 物理学 2016-06-15 F. Marin , R. W. Goosmann , P. -O. Petrucci

We investigate the correlation between infrared (JHKL) and optical (B) fluxes of the variable nucleus of the Seyfert galaxy NGC 4151 using partially published data for the last 6 years (2008-2013.). Here we are using the same data as in…

星系天体物理 · 物理学 2014-11-18 V. L. Oknyansky , N. V. Metlova , O. G. Taranova , V. I. Shenavrin , B. P. Artamonov , C. M. Gaskell , Di-Fu Guo

We have analyzed the two longest (elapsed time > 3 days) BeppoSAX observations of the X-ray brightest Seyfert galaxy, NGC 4151, to search for spectral variability on time-scales from a few tens of ksec to years. We found in both cases…

天体物理学 · 物理学 2008-11-26 S. Puccetti , F. Fiore , G. Risaliti , M. Capalbi , M. Elvis , F. Nicastro , .

We examine the optical photometric and polarimetric variability of the luminous type 1 non-blazar quasar 3C 323.1 (PG 1545+210). Two optical spectro-polarimetric measurements taken during the periods 1996$-$98 and 2003 combined with a…

星系天体物理 · 物理学 2017-01-17 Mitsuru Kokubo

We present an analysis of all SAX observations of NGC 4151. This source was observed 5 times from 1996 to 2001 with durations ranging from a day to four days. The intrinsic continuum, is absorbed at low energies by a complex system: a cold…

天体物理学 · 物理学 2009-11-11 A. De Rosa , L. Piro , G. C. Perola , M. Capalbi , M. Cappi , P. Grandi , L. Maraschi , P. O. Petrucci

We present the results of an intensive ground-based spectrophotometric monitoring campaign of the Seyfert galaxy NGC~4151 for a period of over two months, with a typical temporal resolution of one day. Light curves for four optical…

天体物理学 · 物理学 2009-10-28 S. Kaspi et al

In this paper, we explore the behavior of optical polarization during the multi-wavelength outburst of the blazar Mrk 421 detected in February 2010. We use optical polarization measurements in the wavelength range 500-700 nm from SPOL…

高能天体物理现象 · 物理学 2019-05-29 K K Singh , P J Meintjes , B van Soelen , F A Ramamonjisoa , B Vaidya

AIMS: The main goal of this work is to study possible signs of asymmetry in the bright optical transient in NGC300, with the aim of getting independent information on the explosion mechanism, the progenitor star and its circumstellar…

太阳与恒星天体物理 · 物理学 2015-05-13 F. Patat , J. R. Maund , S. Benetti , M. -T. Botticella , E. Cappellaro , A. Harutyunyan , M. Turatto

We report on the second observing program of the active galactic nucleus NGC 4151 with simultaneous Imaging X-ray Polarimetry Explorer (IXPE; {\sim}750 ks), NuSTAR ({\sim}60 ks), XMM-Newton ({\sim}75 ks), and NICER ({\sim}65 ks) pointings.…

Polarization in stars was first predicted by Chandrasekhar [1] who calculated a substantial linear polarization at the stellar limb for a pure electron-scattering atmosphere. This polarization will average to zero when integrated over a…

太阳与恒星天体物理 · 物理学 2018-04-19 Daniel V. Cotton , Jeremy Bailey , Ian D. Howarth , Kimberly Bott , Lucyna Kedziora-Chudczer , P. W. Lucas , J. H. Hough

Results of the long-term (11 years, from 1996 to 2006) H$\alpha$ and H$\beta$ line variations of the active galactic nucleus of NGC 4151 are presented. High quality spectra (S/N>50 and R~8A) of H$\alpha$ and H$\beta$ were investigated. We…

We investigate the structure of the O-type binary system HD 48099 by measuring linear polarization that arises due to light scattering process. Linear polarization measurements of HD 48099 in the B, V and R passbands with the high-precision…

太阳与恒星天体物理 · 物理学 2016-06-02 A. Berdyugin , V. Piirola , S. Sadegi , S. Tsygankov , T. Sakanoi , M. Kagitani , M. Yoneda , S. Okano , J. Poutanen

We present a polarization variability analysis of a sample of 26 $\gamma$-ray blazars monitored by the Steward Observatory between 2008 and 2018 in the optical band. We investigate the properties and long-term variability of their optical…

We observed the Seyfert 1 galaxy NGC 4151 on eleven occasions at 1-2 day intervals using the Berkeley spectrometer during the ORFEUS-SPAS II mission in 1996 November. The mean spectrum covers 912-1220 A at ~0.3 A resolution with a total…

天体物理学 · 物理学 2009-10-30 B. R. Espey , G. A. Kriss , J. H. Krolik , W. Zheng , Z. Tsvetanov , A. F. Davidsen

Results of a long-term spectral monitoring of the active galactic nucleus of NGC 4151 are presented (11 years, from 1996 to 2006). High quality spectra (S/N>50 in the continuum near Halpha and Hbeta) were obtained in the spectral range…

This study investigates polarimetric characteristics of the blazar 3C~454.3 at 22-129~GHz using decadal~(2011-2022) data sets. In addition, we also delve into the origin of the polarization flare observed in 2019. The data sets were…

The polarized and total flux of the BL Lac object PKS 2155-304 were monitored intensively and simultaneously in the optical UBVRI bands with the Turin photopolarimeter at the CASLEO 2.15 m telescope during 4 campaigns in June, August,…

天体物理学 · 物理学 2009-10-31 Leonardo Tommasi , Ruben Diaz , Eliana Palazzi , Elena Pian , Ennio Poretti , Franco Scaltriti , Aldo Treves

The results of 8-year R-band photopolarimetric data of blazar Mrk 421 collected from February 2008 to May 2016 are presented, along with extensive multiwavelength observations covering from radio to TeV $\gamma$-rays around the flares…

The long-term optical and near infrared monitoring observations for a type 1 act ive galactic nucleus NGC 4151 were carried out for six years from 2001 to 2006 b y using the MAGNUM telescope, and delayed response of flux variations in the…

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