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Self-broadening in Balmer line wing formation in stellar atmospheres
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Department of Physics and Astronomy, Observational Astronomy.
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Department of Physics and Astronomy, Observational Astronomy.
2000 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 363, no 3, 1091-1105 p.Article in journal (Refereed) Published
Place, publisher, year, edition, pages
2000. Vol. 363, no 3, 1091-1105 p.
Keyword [en]
atomic processes; line : profiles; stars : atmospheres; NEUTRAL HYDROGEN-ATOMS; COOL DWARF STARS; MODEL ATMOSPHERES; SPECTRAL-LINES; A-STAR; F-STAR; COLLISIONS; TRANSITIONS; CONVECTION; ABUNDANCE
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URN: urn:nbn:se:uu:diva-36621OAI: oai:DiVA.org:uu-36621DiVA: diva2:64520
Available from: 2007-01-09 Created: 2007-01-09 Last updated: 2011-01-14

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Barklem, PaulPiskunov, Nikolai

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