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Related papers: HUT Observations of Time-Variable Absorption in NG…

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We present the results of a recent (March 2011) 160 ks Chandra-LETGS observation of the Seyfert galaxy NGC 4593, and the analysis of archival X-ray and UV spectra taken with XMM-Newton and HST/STIS in 2002. We find evidence of a…

High Energy Astrophysical Phenomena · Physics 2015-06-16 J. Ebrero , J. S. Kaastra , G. A. Kriss , C. P. de Vries , E. Costantini

The Seyfert 1 galaxy 1H 0419-577 hosts a $\sim$kpc extended outflow that is evident in the [\ion{O}{iii}] image and that is also detected as a warm absorber in the UV/X-ray spectrum. Here, we analyze a $\sim$30 ks Chandra-ACIS X-ray image,…

High Energy Astrophysical Phenomena · Physics 2017-12-13 L. Di Gesu , E. Costantini , E. Piconcelli , J. S. Kaastra , M. Mehdipour , S. Paltani

We present a detailed study of AGN feedback in the narrow-line region (NLR) of the Seyfert 1 galaxy NGC 4151. We illustrate the data and techniques needed to determine the mass outflow rate and kinetic luminosity of the outflowing ionized…

Astrophysics of Galaxies · Physics 2015-06-23 D. M. Crenshaw , T. C. Fischer , S. B. Kraemer , H. R. Schmitt

The emission and absorption attributes of the UV-blue nuclear spectra of the Narrow-Line Seyfert 1 (NLS1) galaxies are analyzed based on high quality archival HST observations. Measurements from composite spectra as well as from individual…

Astrophysics · Physics 2007-05-23 Anca Constantin , Joseph C. Shields

We present the first results of the Hubble Space Telescope/Faint Object Camera long-slit spectroscopy of the inner 8" of the Narrow Line Region of NGC 4151 at a spatial resolution of 0".029. The emission gas is characterized by an…

Astrophysics · Physics 2015-06-24 Claudia Winge , D. J. Axon , F. D. Macchetto , A. Capetti

Methods. We analyse two observations taken with the Low Energy Transmission Grating Spectrometer of Chandra. We investigated the spectral response to a sudden flux decrease by a factor of 5, which occurred during the second observation.…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-13 K. C. Steenbrugge , M. Fenovcik , J. S. Kaastra , E. Costantini , F. Verbunt

One of the outstanding problems of current observational cosmology is to understand the nature of sources that produced the bulk of the ionizing radiation after the Cosmic Dark Age. Direct detection of these reionization sources is…

We present observations of the UV absorption lines in the luminous Seyfert 1 galaxy Mrk 509, obtained with the medium resolution (lambda/Delta-lambda ~ 40,000) echelle gratings of the Space Telescope Imaging Spectrograph on the Hubble Space…

We report the detection of variable UV absorption lines in NGC 4395, based on UV observations with the HST STIS carried out in April and July, 2004, as part of a reverberation-mapping campaign. Low-ionization lines of O I, N I, Si II, C II,…

Astrophysics · Physics 2013-04-22 Alexei Baskin , Ari Laor

We analyze spectra of a gravitationally lensed galaxy, known as the Sunburst Arc, that is leaking ionizing photons, also known as the Lyman continuum (LyC). Magnification from gravitational lensing permits the galaxy to be spatially…

High resolution X-ray spectroscopy is a powerful tool for studying the nature of the matter surrounding the neutron star in X-ray binaries and its interaction between the stellar wind and the compact object. In particular, absorption…

High Energy Astrophysical Phenomena · Physics 2016-08-11 J. J. Rodes-Roca , J. M. Torrejón , S. Martínez-Núñez , A. Giménez-García , G. Bernabéu

We present a study of 7 star-forming galaxies from the Cosmic Evolution Survey (COSMOS) observed with the Cosmic Origins Spectrograph (COS) on board the Hubble Space Telescope (HST). The galaxies are located at relatively low redshifts,…

Low mass, low metallicity galaxies at low to moderate ($z\lesssim3$) redshifts offer the best opportunity for detailed examination of the interplay between massive stars, ionizing radiation and gas in sources similar to those that likely…

Astrophysics of Galaxies · Physics 2019-10-16 Dawn K. Erb , Danielle A. Berg , Matthew W. Auger , David L. Kaplan , Gabriel Brammer , Max Pettini

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 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…

Astrophysics · Physics 2007-05-23 Stefanie Komossa , Henner Fink

We present an analysis of the intrinsic UV absorption in the Seyfert 1 galaxy Mrk 279 based on simultaneous long observations with the Hubble Space Telescope (41 ks) and the Far Ultraviolet Spectroscopic Explorer (91 ks). To extract the…

In this paper we analyze the X-ray, UV and optical data of the Seyfert 1.5 galaxy 1H0419-577, with the aim of detecting and studying an ionized-gas outflow. The source was observed simultaneously in the X-rays with XMM and in the UV with…

High Energy Astrophysical Phenomena · Physics 2015-06-16 L. Di Gesu , E. Costantini , N. Arav , B. Borguet , R. G. Detmers , J. Ebrero , D. Edmonds , J. S. Kaastra , E. Piconcelli , F. Verbunt

All far ultraviolet observations of HD209458 tend to support a scenario in which the inflated hydrogen atmosphere of its planetary companion strongly absorbs the stellar \lya flux during transit. However, it was not clear how the transit…

Astrophysics · Physics 2009-11-13 Lotfi Ben-Jaffel

We discuss the power of time-evolving photoionization as a diagnostic tool to measure the electron density of photoionized gas. We apply this technique to a XMM-Newton observation of the ionized absorber in the Seyfert 1 galaxy NGC 4051,…

In this paper we present the analysis of two broad band (0.1-150 keV) BeppoSAX observations of the Seyfert 1 galaxy NGC 3516. The two observations were taken 4 months apart, on 1996 November 8 and 1997 March 12 respectively. We report a…