OH eruptive Mira stars.

Details OH eruptive Mira stars. OH eruptive Mira stars.

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...321..877e&link_type=abstract

Astronomy and Astrophysics, v.321, p.877-887

Astronomy and Astrophysics

Astrophysics

15

Stars: Agb, Post-Agb, Radio Lines: Stars, Stars: Individual: R Leo, U Her, R Cnc, R Lmi

Scientific paper

We report the evolution of new OH flares detected from four Miras. These eruptive stars possess in common the fact that they have very thin envelopes. Except for one of them, each eruptive feature has a velocity near that of the star. Preferentially, the eruptive lines are at 1612 and 1665MHz. It is likely that OH flares take place in a zone of the envelope closer to the star than standard emission.

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