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HD 174884: a strongly eccentric, short-period early-type binary system discovered by CoRoT

Publication at Faculty of Mathematics and Physics |
2009

Abstract

Accurate CoRoT space photometry and follow up high dispersion spectroscopy led to the discovery that HD 174884 is a young eclipsing and double-lines spectroscopic binary with a period of 3.657 days and an eccentric orbit ( e=0.3).The secondary eclipse is only 0.0015 mag.deep and the system consists of two late B stars.