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Resolving Stellar Atmospheres 1. Hα line and comparisons to microlensing observations

Thurl, Christine; Sackett, Penny; Hauschildt, Peter H


Context. We present work on Hα spectral line characteristics in PHOENIX stellar model atmospheres and their comparison to microlensing observations. Aims. We examine in detail the Ha equivalent width (EW) and the line shape characteristics for effective

CollectionsANU Research Publications
Date published: 2006
Type: Journal article
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361:20054766


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