OH Infrared Stars - Very Long Period Variables with Enormous Mass Loss

Details OH Infrared Stars - Very Long Period Variables with Enormous Mass Loss OH Infrared Stars - Very Long Period Variables with Enormous Mass Loss

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981msngr..24...24e&link_type=abstract

The Messenger, No.24, P. 24, 1981

Astronomy and Astrophysics

Astronomy

Scientific paper

Since 1975 infrared photometers attached to the ESO 1m telescape have been used to investigate OH/IR stars. Monitoring them over five years, G. V. Schultz and W. A. Sherwood from the Max-Planck-Institut für Radioastronomie in Bann and the author proved that OH/IR stars are lang period variables, which in extreme cases have periods langer than four years.

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