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We report the discovery of rapid variations of a high-velocity Mg ii broad absorption line (BAL) trough in the quasar SDSS J133356.02+001229.1 (zem ~ 0.9197). Vivek et al. (2012a) revealed the emergence and subsequent near disappearance of…

Astrophysics of Galaxies · Physics 2018-10-17 M. Vivek , R. Srianand , K. S. Dawson

Three Galactic O-type stars belong to the rare class of Of?p objects: HD108, HD191612, and HD148937. The first two stars show a wealth of phenomena, including magnetic fields and strong X-ray emission, light variability, and dramatic…

Astrophysics · Physics 2009-11-13 Y. Naze , N. R. Walborn , G. Rauw , F. Martins , A. M. T. Pollock , H. E. Bond

We present an analysis of the rms variability spectra of a sample of 18 observations of 14 Seyfert galaxies observed by XMM-Newton, which exhibit sufficient variability and signal-to-noise ratio to examine the variations in the iron K-band.…

Cosmology and Nongalactic Astrophysics · Physics 2016-03-02 Shyam Bhayani , Kirpal Nandra

We examine archival XMM-Newton data on the extremely variable narrow-line Seyfert 1 (NLS1) active galactic nucleus (AGN) 1H 0707-495. We construct fractional excess variance (Fvar) spectra for each epoch, including the recent 2019…

High Energy Astrophysical Phenomena · Physics 2021-09-08 M. L. Parker , W. N. Alston , L. Härer , Z. Igo , A. Joyce , D. J. K. Buisson , P. Chainakun , A. C. Fabian , J. Jiang , P. Kosec , G. A. Matzeu , C. Pinto , Y. Xu , F. Zaidouni

In order to examine how narrow emission-line flux ratios depend on the Seyfert type, we compiled various narrow emission-line flux ratios of 355 Seyfert galaxies from the literature. We present in this paper that the intensity of the…

Astrophysics · Physics 2015-06-24 Tohru Nagao , Takashi Murayama , Yoshiaki Taniguchi

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…

Astrophysics · Physics 2009-10-30 B. R. Espey , G. A. Kriss , J. H. Krolik , W. Zheng , Z. Tsvetanov , A. F. Davidsen

This paper presents a quantification of the X-ray variability amplitude for 79 ASCA observations of 36 Seyfert 1 galaxies. We find that consideration of sources with the narrowest permitted lines in the optical band introduces scatter into…

Astrophysics · Physics 2009-10-31 T. J. Turner , I. M. George , K. Nandra , D. Turcan

High resolution X-ray spectroscopy of the warm absorber in the nearby X-ray bright Seyfert 1 galaxy, Mrk 1040 is presented. The observations were carried out in the 2013-2014 timeframe using the Chandra High Energy Transmission Grating with…

High Energy Astrophysical Phenomena · Physics 2017-03-08 James Reeves , Valentina Braito , Ehud Behar , Travis Fischer , Steve Kraemer , Andrew Lobban , Emanuele Nardini , Delphine Porquet , Jane Turner

For 3 radio-loud $\gamma$-ray detected Narrow-Line Seyfert 1 ($\gamma$-ray NLSy1) galaxies, we report optical variability on intra-night and/or week-like time scales, based on five $\geq$ 3 hours long monitoring sessions for each galaxy.…

Astrophysics of Galaxies · Physics 2018-12-12 Vineet Ojha , Gopal-Krishna , Hum Chand

We model the broad emission lines present in the optical, UV and X-ray spectra of Mrk 509, a bright type 1 Seyfert galaxy. The broad lines were simultaneously observed during a large multiwavelength campaign, using the XMM-Newton-OM for the…

We report optical, soft X-ray, and UV observations of the peculiar Seyfert galaxy IC 3599 using data obtained with ROSAT and IUE. Most remarkably, we discovered a rapid decrease of the X-ray flux by a factor of about 100 within one year and…

Astrophysics · Physics 2007-05-23 D. Grupe , K. Beuermann , K. Mannheim , N. Bade , H. -C. Thomas , D. de Martino , A. Schwope

Following the recent discovery of gamma rays from the radio-loud narrow-line Seyfert 1 galaxy PMN J0948+0022 (z=0.5846), we started a multiwavelength campaign from radio to gamma rays, which was carried out between the end of March and the…

The narrow-line Seyfert 1 galaxy IRAS 07598+6508 is known to be a stong Fe II emitter. The analysis of several high S/N ratio spectra shows that its spectrum is dominated by a relatively narrow "broad line" region (1 780 km s$^{-1}$ FWHM)…

Astrophysics · Physics 2009-11-11 M. -P. Veron , M. Joly , P. Veron , T. Boroson , S. Lipari , P. Ogle

We examine the variability in the intrinsic absorption in the Seyfert 1 galaxy Mrk 279 using three epochs of observations from the Far Ultraviolet Spectroscopic Explorer (FUSE) and two epochs of observations with the Space Telescope Imaging…

We present the results of our broadband study of the $\gamma$-ray emitting narrow line Seyfert 1 (NLSy1) galaxy SBS 0846+513 ($z=0.585$). This includes multi-band flux variations, $\gamma$-ray spectral analysis, broad band spectral energy…

High Energy Astrophysical Phenomena · Physics 2016-03-23 Vaidehi S. Paliya , Bhoomika Rajput , C. S. Stalin , S. B. Pandey

Context. Plaskett's star (HD47129) is a very massive O-star binary in a post Roche-lobe overflow stage. CoRoT observations of this system revealed photometric variability with a number of frequencies. Aims. The aim of this paper is to…

Solar and Stellar Astrophysics · Physics 2015-06-23 Matthieu Palate , Gregor Rauw

We present an analysis of spectrum and variability of the bright reddened narrow line Seyfert 1 galaxy Was~61 using 90 ks archival {\it XMM-Newton} data. The X-ray spectrum in 0.2-10 keV can be characterized by an absorbed power-law plus…

High Energy Astrophysical Phenomena · Physics 2016-03-11 Liming Dou , Ting-Gui Wang , Yanli Ai , Weimin Yuan , Hongyan Zhou , Xiao-Bo Dong

During an extensive multiwavelength campaign that we performed in 2013-14 the prototypical Seyfert 1 galaxy NGC 5548 has been found in an unusual condition of heavy and persistent obscuration. The newly discovered "obscurer" absorbs most of…

We present strong evidence for variability of the flux of the iron K$\alpha$ emission line in the Seyfert 1 galaxy, NGC 3516. Two ASCA observations, separated by $\sim 1$~yr, showed a marked decrease in continuum flux by $\sim 60$~per cent.…

Astrophysics · Physics 2016-01-13 K. Nandra , R. F. Mushotzky , T. Yaqoob , I. M. George , T. J. Turner