Author： Bonanos Alceste Z. Spetsieri Zoi T. Gavras Panagiotis Bonanos Alceste Z. Bonanos Alceste Z. Bonanos Alceste Z. Bonanos Alceste Z. Bonanos Alceste Z. Bonanos Alceste Z. Bonanos Alceste Z.
Publisher： Edp Sciences
E-ISSN： 1432-0746|616|issue|A175-A175
ISSN： 0004-6361
Source： Astronomy & Astrophysics, Vol.616, Iss.issue, 2018-09, pp. : A175-A175
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
Related content
Access to resources
Recommend
An estimate of the structural parameters of the Large Magellanic Cloud using red clump stars
By Subramanian S. Subramaniam A.
Astronomy & Astrophysics, Vol. 520, Iss. issue, 2010-09 ,pp. :
Spatially resolved dusty torus toward the red supergiant WOH G64 in the Large Magellanic Cloud
Astronomy & Astrophysics, Vol. 484, Iss. 2, 2008-06 ,pp. :
Chemically peculiar stars in the Large Magellanic Cloud
Astronomy & Astrophysics, Vol. 459, Iss. 3, 2006-12 ,pp. :
Massive runaway stars in the Large Magellanic Cloud
By Gvaramadze V. V. Kroupa P. Pflamm-Altenburg J.
Astronomy & Astrophysics, Vol. 519, Iss. issue, 2010-09 ,pp. :