Physical Parameters of the Massive Multiple System Eta-Orionis

Details Physical Parameters of the Massive Multiple System Eta-Orionis Physical Parameters of the Massive Multiple System Eta-Orionis

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.142...99w&link_type=abstract

Astrophysics and Space Science, Volume 142, Issue 1-2, pp. 99-101

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The bright massive object η Orionis is at the same time a totally eclipsing system, a spectroscopic triple system, a speckle triple system and a visual binary. These circumstances offer an exceptional opportunity for determining the physical parameters of massive stars. The authors' observations show that the published elements are wrong. They present a new determination of several parameters of the multiple system and propose new visual observations.

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