The Broadering of Spectral Lines by Collisions with Neutral Hydrogen Atoms in Cool Stars

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The Broadering of Spectral Lines by Collisions with Neutral Hydrogen Atoms in Cool Stars

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dc.contributor.author Barklem, Paul
dc.contributor.editor Popović, Luka Č.
dc.date.accessioned 2011-01-10T10:06:49Z
dc.date.available 2011-01-10T10:06:49Z
dc.date.issued 2007
dc.identifier.isbn 978-86-80019-17-8 en_US
dc.identifier.uri http://hdl.handle.net/123456789/1449
dc.description.provenance Submitted by Slavisha Milisavljevic (slavisha) on 2011-01-10T10:06:49Z No. of bitstreams: 1 I01.pdf: 4442259 bytes, checksum: dfd2d6a4f5bbc30999a47aed7ca33a8e (MD5) en
dc.description.provenance Made available in DSpace on 2011-01-10T10:06:49Z (GMT). No. of bitstreams: 1 I01.pdf: 4442259 bytes, checksum: dfd2d6a4f5bbc30999a47aed7ca33a8e (MD5) Previous issue date: 2007 en
dc.language.iso en en_US
dc.publisher Nenad Milovanović & Milan S. Dimitrijević, Astronomical Observatory, Belgrade en_US
dc.title The Broadering of Spectral Lines by Collisions with Neutral Hydrogen Atoms in Cool Stars en_US
mf.subject.keywords I will review the theory of broadening of metallic spectral lines by neutral hydrogen atom collisions developed by Anstee, Barklem and O'Mara. I will discuss why the theory works, while able to retain the wide range of applicability needed for astrophysical applications. I will discuss the present status of large scale calculations for many spectral lines for neutral and singly ionised species. Some examples of application to analysis of cool star spectra will be discussed. Time permitting, the extension of the theory to self broadening of hydrogen lines will be discussed briefly. en_US
mf.document.pages 24 en_US
mf.contributor.editor-in-chief Dimitrijević, S. Milan

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