| 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 |
|