Photographische Beobachtung des roten Sterns V447 Ophiuchi.

Details Photographische Beobachtung des roten Sterns V447 Ophiuchi. Photographische Beobachtung des roten Sterns V447 Ophiuchi.

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mitvs..12...88r&link_type=abstract

Mitt. Veränderliche Sterne, Band 12, Heft 5, p. 88

Physics

Scientific paper

The star proves to be a semiregular variable with a cycle length varying
between 105 and 155 days.

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