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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
Abstract
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
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- Copyright © Astronomical Society of the Pacific 2001