Possibility that the Far Ultraviolet Excess in M31 is Due to Main-Sequence Stars

Details Possibility that the Far Ultraviolet Excess in M31 is Due to Main-Sequence Stars Possibility that the Far Ultraviolet Excess in M31 is Due to Main-Sequence Stars

Dec 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971a%26a....15..403t&link_type=abstract

Astronomy and Astrophysics, Vol. 15, p. 403 (1971)

Astronomy and Astrophysics

Astrophysics

9

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1971A&A....15..403T

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