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Related papers: Reconciling X-ray and 21cm HI absorption gas colum…

200 papers

We have used the Arecibo telescope to carry out an survey of 31 dark clouds in the Taurus/Perseus region for narrow absorption features in HI ($\lambda$ 21cm) and OH (1667 and 1665 MHz) emission. We detected HI narrow self--absorption…

Astrophysics · Physics 2009-11-07 Di Li , Paul F. Goldsmith

Combining our own observations with data from the literature, we consider the incidence of HI absorption in Gigahertz Peaked Spectrum (GPS) and Compact Steep Spectrum (CSS) sources. Here we present our preliminary results, where we find…

Astrophysics · Physics 2009-11-07 Y. M. Pihlstroem , J. E. Conway , R. C. Vermeulen

We report on a survey for associated HI 21-cm and OH 18-cm absorption with the Giant Metrewave Radio Telescope at redshifts z = 0.2-0.4. Although the low redshift selection ensures that our targets are below the critical ultra-violet…

Astrophysics of Galaxies · Physics 2017-03-29 S. J. Curran , M. T. Whiting , J. R. Allison , A. Tanna E. M. Sadler , R. Athreya

We have searched for evidence of soft X-ray absorption by hot metals in the vicinity of the Galaxy in the spectra of a small sample of fifteen Type I AGN observed with the high resolution X-ray gratings on board Chandra. This is an…

Astrophysics · Physics 2009-11-11 B. McKernan , T. Yaqoob , C. S. Reynolds

We present results from MUSE observations of a 21-cm HI absorption system detected with the Australian Square Kilometre Array Pathfinder radio telescope at redshift $z = 0.4503$ towards the $z = 1.71$ quasar PKS 1610-771. We identify four…

We present the results of optical spectroscopic identifications of a bright subsample of 2-10keV hard X-ray selected sources from the ASCA Medium Sensitivity Survey in the northern sky. The flux limit of the subsample is 3*10^-13 erg s^-1…

Astrophysics · Physics 2009-11-10 Masayuki Akiyama , Yoshihiro Ueda , Kouji Ohta , Tadayuki Takahashi , Toru Yamada

We present a large compilation of reddening estimates from broad-line Balmer decrements for active galactic nuclei (AGNs) with measured X-ray column densities. The median reddening is E(B-V) ~ 0.77 +/- 0.10 for type-1 to type-1.9 AGNs with…

Astrophysics of Galaxies · Physics 2021-12-14 Gunnar W. Jaffarian , C. Martin Gaskell

We remark on the utility of an observational relation between the absorption column density in excess of the Galactic absorption column density, $\Delta N_{\rm H} = N_{\rm H, fit} - N_{\rm H, gal}$, and redshift, z, determined from all 55…

We characterise the relation between the gas and dust content of the interstellar medium towards young stellar objects in the Orion Nebula Cluster. X-ray observations provide estimates of the absorbing equivalent hydrogen column density N_H…

Solar and Stellar Astrophysics · Physics 2016-08-31 Birgit Hasenberger , Jan Forbrich , Joao Alves , Scott Wolk , Stefan Meingast , Konstantin Getman , Ignazio Pillitteri

In this paper we study 21-cm absorption spectra and the corresponding emission spectra toward bright continuum sources in the test region (326deg< l < 333 deg) of the Southern Galactic Plane Survey. This survey combines the high resolution…

Astrophysics · Physics 2009-11-07 John M. Dickey , N. M. McClure-Griffiths , B. M. Gaensler , A. J. Green

We review some of the main physical and statistical properties of the X-ray absorber in AGNs. In particular, we review the distribution of the absorbing column density inferred from X-ray observations of various AGN samples. We discuss the…

Astrophysics · Physics 2007-05-23 R. Maiolino , G. Risaliti

We present a 21-cm emission-absorption study towards extragalactic sources in the Canadian Galactic Plane Survey (CGPS). We have analyzed HI spectra towards 437 sources with S > 150 mJy, giving us a source density of 0.6 sources per square…

Astrophysics · Physics 2009-11-10 S. T. Strasser , A. R. Taylor

(Abridged) We present Herschel/HIFI spectra of the H2O 1113 GHz and H2O+ 1115 GHz lines toward five nearby prototypical starburst/AGN systems, and OH+ 971 GHz spectra toward three of these. The beam size of 20" corresponds to resolutions…

Astrophysics of Galaxies · Physics 2016-09-14 Floris van der Tak , Axel Weiss , Lijie Liu , Rolf Guesten

This paper considers some effects of foreground Galactic gas on radiation received from extragalactic objects, with an emphasis on the use of the 21cm line to determine the total N(HI). In general, the opacity of the 21cm line makes it…

Astrophysics · Physics 2016-01-27 Felix J. Lockman

We investigate the relation between the optical extinction ($A_V$) and the hydrogen column density ($N_H$) determined from X-ray observations of a large sample of Galactic sightlines toward 35 supernova remnants, 6 planetary nebulae, and 70…

Astrophysics of Galaxies · Physics 2017-08-30 Hui Zhu , Wenwu Tian , Aigen Li , Mengfei Zhang

We report the results of a survey for HI 21-cm absorption at z < 0.4 in a new sample of radio sources with the Giant Metrewave Radio Telescope. Of the 11 sources for which there are good data, we obtain zero detections, where four are…

Astrophysics of Galaxies · Physics 2019-01-16 S. J. Curran , R. W. Hunstead , H. M. Johnston , M. T. Whiting , E. M. Sadler , J. R. Allison , R. Athreya

We present the results of a survey for HI 21-cm and OH 18-cm absorption in seven strong CO emitters at z > 3. Despite reaching limits comparable to those required to detect 21-cm absorption at lower redshifts, we do not detect either…

Astrophysics of Galaxies · Physics 2016-03-16 S. J. Curran , J. R. Allison , M. T. Whiting , E. M. Sadler , F. Combes , M. B. Pracy , C. Bignell , R. Athreya

We report the detection of HI absorption towards the inner double of the double-double radio galaxy (DDRG) J1247+6723 with the Giant Metrewave Radio Telescope (GMRT). The inner double is a Giga-hertz peaked spectrum (GPS) source with a…

Astrophysics · Physics 2008-11-26 D. J. Saikia , Neeraj Gupta , C. Konar

We present an overview of the occurrence and properties of atomic gas associated with compact radio sources at redshifts up to z=0.85. Searches for HI 21cm absorption were made with the Westerbork Synthesis Radio Telescope at UHF-high…

We present a method for the identification of heavily absorbed AGN (NH>10^23 cm^-2) from X-ray photometric data. We do this using a set of XMM-Newton reference spectra of local galaxies for which we have accurate NH information, as…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Murray Brightman , Kirpal Nandra