An empirical method to estimate the LMC distance using B-stars in eclipsing binary systems
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20011528/pdf
Reference25 articles.
1. An Empirical Procedure to Estimate Distances to Stellar Clusters
2. Accurate masses and radii of normal stars
3. Stellar Angular Diameters and Visual Surface Brightness -- I LATE SPECTRAL TYPES
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1. A PROBLEM WITH THE CLUSTERING OF RECENT MEASURES OF THE DISTANCE TO THE LARGE MAGELLANIC CLOUD;The Astronomical Journal;2007-12-07
2. Eclipsing Binaries in the MACHO Database: New Periods and Classifications for 3031 Systems in the Large Magellanic Cloud;The Astrophysical Journal;2007-07
3. The Pleiades eclipsing binary HD 23642 revisited;Astronomy & Astrophysics;2006-11-13
4. Eclipsing binaries as standard candles;Astronomy & Astrophysics;2004-12-17
5. Improved Baade-Wesselink surface brightness relations;Monthly Notices of the Royal Astronomical Society;2004-08-23
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