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An Analysis of HST/FOS Spectra of Spatially Resolved Compact OB Systems in the LMC

Published online by Cambridge University Press:  13 May 2016

E. Niemczura  and
H. Cugier
E. Niemczura
Affiliation:
Astronomical Institute of the Wroclaw University, ul. Kopernika 11, 51-622 Wroclaw, Poland
H. Cugier
Affiliation:
Astronomical Institute of the Wroclaw University, ul. Kopernika 11, 51-622 Wroclaw, Poland

Abstract

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An analysis of the spatially resolved (0.1) main-sequence stars of four compact multiple systems located in the Large Magellanic Cloud (LMC) is given. For this purpose we compared theoretical synthetic spectra with the observations obtained by means of the Faint Object Spectrograph (FOS) aboard the Hubble Space Telescope (HST).

Type
Stars and Stellar Atmospheres
Information
Symposium - International Astronomical Union , Volume 205: Galaxies and their Constituents at the Highest Angular Resolutions , 2001 , pp. 312 - 313
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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