AF Ari - Ein heller Bedeckungsveraenderlicher mit einem G-Riesen

Details AF Ari - Ein heller Bedeckungsveraenderlicher mit einem G-Riesen AF Ari - Ein heller Bedeckungsveraenderlicher mit einem G-Riesen

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011bavsr..60..150h&link_type=abstract

BAV Rundbrief 3/2011, vol. 60, p. 150-152

Computer Science

Eclipsing Binary

Scientific paper

By combining existing and including new photometric data a first solution can now be presented: AF Ari is a well detached binary having an eccentric orbit and a period of 153 days. The secondary component is identified as an A-type dwarf. The mass of the G-type giant is estimated at 2.65 solar masses. Apparently, AF Ari is a new z (zeta) Aurigae type system and suited for double-lined spectroscopy. The english version of the article will be found behind the german version.

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