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Optical Spectroscopy of HD102567 (4U1145-61)
Published online by Cambridge University Press: 14 August 2015
Abstract
Analysis of optical spectra of HD102567 (HEN 715), the optical counterpart of the X-ray source 4U1145-61 is presented. Estimates of the star's rotation velocity, inclination angle, distance and envelope characteristics are given. Some consequences of the possible existence of a 190d orbital period for this Be/X-ray sources are discussed.
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- III. Spectroscopy
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- Copyright © Reidel 1982
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