An OH maser towards the globular cluster NGC 6171

Details An OH maser towards the globular cluster NGC 6171 An OH maser towards the globular cluster NGC 6171

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...287l..29f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 287, no. 2, p. L29-L30

Astronomy and Astrophysics

Astronomy

2

Globular Clusters, Infrared Astronomy, Interstellar Masers, Mira Variables, Asymptotic Giant Branch Stars, Infrared Photometry, Stellar Luminosity

Scientific paper

The Mira variable, V720 Oph is a newly discovered OH-maser and possible
member of the globular cluster NGC 6171. Infrared photometry of this
star suggests that if it is indeed a member of the cluster its
luminosity is significantly greater than normally reached by low mass
Asymptotic Giant Branch (AGB) stars.

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