SIMBAD references

1997A&A...321..877E - Astronomy and Astrophysics, volume 321, 877-887 (1997/5-3)

OH eruptive Mira stars.


Abstract (from CDS):

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.

Abstract Copyright:

Journal keyword(s): stars: AGB, post-AGB - radio lines: stars - stars: individual: R Leo, U Her, R Cnc, R LMi

Simbad objects: 18

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:1997A&A...321..877E and select 'bookmark this link' or equivalent in the popup menu


© Université de Strasbourg/CNRS

    • Contact