Resolving Stellar Atmospheres 1. Hα line and comparisons to microlensing observations
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
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
|01_Thurl_Resolving_Stellar_Atmospheres_2006.pdf||596.73 kB||Adobe PDF||Request a copy|
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