Brey 73 - A multiple Wolf-Rayet star

Details Brey 73 - A multiple Wolf-Rayet star Brey 73 - A multiple Wolf-Rayet star

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988msngr..54...43t&link_type=abstract

ESO Messenger (ISSN 0722-6691), Dec. 1988, p. 43-47.

Computer Science

10

Stellar Spectrophotometry, Stellar Systems, Wolf-Rayet Stars, Charge Coupled Devices, Magellanic Clouds, Stellar Evolution, Stellar Luminosity, Stellar Magnitude

Scientific paper

CCD images of the WR star Brey 73 were obtained with a 2.2-m telescope
in October, 1987. The CAPELLA software package for profile fitting
photometry (Debray et al., 1988) was used. The results show that Brey 73
is an aggregate of 11 components. The apparent and absolute magnitudes
of the aggregate are determined.

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