Massive Early-Type Emission-Line Stars: an Attempt to Distinguish a New Group of Stellar Objects

Details Massive Early-Type Emission-Line Stars: an Attempt to Distinguish a New Group of Stellar Objects Massive Early-Type Emission-Line Stars: an Attempt to Distinguish a New Group of Stellar Objects

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..519m&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 519-520

Astronomy and Astrophysics

Astrophysics

2

Emission Line Stars, Supergiants, Binaries

Scientific paper

A new sample of possibly massive early-type emission-line stars (METELS) based on the previous lists of peculiar Be stars is presented. It consists of 36 objects divided amongst supergiants, possible binaries, and candidates to the list. The central stars are probably more massive than ˜ 10M &sun;. Two new relations allowing idientification of possible binaries among the objects are proposed.

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