Skip navigation
Skip navigation

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

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

Description

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
URI: http://hdl.handle.net/1885/18334
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361:20054766

Download

File Description SizeFormat Image
01_Thurl_Resolving_Stellar_Atmospheres_2006.pdf596.73 kBAdobe PDF    Request a copy


Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  12 November 2018/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator