A comparison of metal and Ly-α absorption in galactic haloes

The metallicity structure of galactic haloes is one of the major unknowns in modern galactic astrophysics and observational cosmology. Hereby we outline a very simple method for obtaining at least a crude picture of gas abundances, based on recent important statistical determination of the...

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Main Author: Ćirković M.M.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 1998-01-01
Series:Serbian Astronomical Journal
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/1998/1450-698X9858009C.pdf
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author Ćirković M.M.
author_facet Ćirković M.M.
author_sort Ćirković M.M.
collection DOAJ
description The metallicity structure of galactic haloes is one of the major unknowns in modern galactic astrophysics and observational cosmology. Hereby we outline a very simple method for obtaining at least a crude picture of gas abundances, based on recent important statistical determination of the relationship between neutral hydrogen absorbing column density and galaxy impact parameter. It is a fine illustration of the great theoretical and observational power of low-redshift Lyα absorption studies. Future detailed analyses of large samples of absorption-selected galaxies will certainly provide us with more data on the abundance structure of extended gaseous component of galaxies.
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spelling doaj.art-961ea622a99244759814ea8c8828f4462022-12-21T22:38:12ZengAstronomical Observatory, Department of Astronomy, BelgradeSerbian Astronomical Journal1450-698X1820-92891998-01-01199815891310.2298/SAJ9858009C1450-698X9858009CA comparison of metal and Ly-α absorption in galactic haloesĆirković M.M.0Astronomical Observatory, Belgrade + Astronomy Program, Department of Physics and Astronomy State University of New York at Stony Brook, Stony Brook, NY, USAThe metallicity structure of galactic haloes is one of the major unknowns in modern galactic astrophysics and observational cosmology. Hereby we outline a very simple method for obtaining at least a crude picture of gas abundances, based on recent important statistical determination of the relationship between neutral hydrogen absorbing column density and galaxy impact parameter. It is a fine illustration of the great theoretical and observational power of low-redshift Lyα absorption studies. Future detailed analyses of large samples of absorption-selected galaxies will certainly provide us with more data on the abundance structure of extended gaseous component of galaxies.http://www.doiserbia.nb.rs/img/doi/1450-698X/1998/1450-698X9858009C.pdf
spellingShingle Ćirković M.M.
A comparison of metal and Ly-α absorption in galactic haloes
Serbian Astronomical Journal
title A comparison of metal and Ly-α absorption in galactic haloes
title_full A comparison of metal and Ly-α absorption in galactic haloes
title_fullStr A comparison of metal and Ly-α absorption in galactic haloes
title_full_unstemmed A comparison of metal and Ly-α absorption in galactic haloes
title_short A comparison of metal and Ly-α absorption in galactic haloes
title_sort comparison of metal and ly α absorption in galactic haloes
url http://www.doiserbia.nb.rs/img/doi/1450-698X/1998/1450-698X9858009C.pdf
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