Variability of massive stars with known spectral types in the Small Magellanic Cloud using 8 years of OGLE-III data-Reference-Cited by-同舟云学术

Variability of massive stars with known spectral types in the Small Magellanic Cloud using 8 years of OGLE-III data

Published:2014-02 Issue: Volume:562 Page:A125
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Kourniotis M.,Bonanos A. Z.,Soszyński I.,Poleski R.,Krikelis G.,Udalski A.,Szymański M. K.,Kubiak M.,Pietrzyński G.,Wyrzykowski Ł.,Ulaczyk K.,Kozłowski S.,Pietrukowicz P.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201322856/pdf

Reference95 articles.

1. DUSTY OB STARS IN THE SMALL MAGELLANIC CLOUD. II. EXTRAGALACTIC DISKS OR EXAMPLES OF THE PLEIADES PHENOMENON?

2. Possible gravitational microlensing of a star in the Large Magellanic Cloud

3. Accurate masses and radii of normal stars

4. Using Cepheids to determine the galactic abundance gradient

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