Star formation history and X-ray binary populations: the case of the Large Magellanic Cloud
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/459/1/528/8113354/stw167.pdf
Reference207 articles.
1. A review of the distance and structure of the Large Magellanic Cloud
2. Abundances of the elements: Meteoritic and solar
3. THECHANDRASURVEY OF THE SMALL MAGELLANIC CLOUD “BAR”. II. OPTICAL COUNTERPARTS OF X-RAY SOURCES
4. OPTICAL SPECTROSCOPY OF 20 Be/X-RAY BINARIES IN THE SMALL MAGELLANIC CLOUD
5. STAR FORMATION HISTORY AND X-RAY BINARY POPULATIONS: THE CASE OF THE SMALL MAGELLANIC CLOUD
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