The eclipsing binary system HD208496

Details The eclipsing binary system HD208496 The eclipsing binary system HD208496

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...74..247v&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 74, no. 2, Aug. 1988, p. 247-250.

Astronomy and Astrophysics

Astrophysics

3

Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Electrophotometry, Main Sequence Stars, Stellar Magnitude, Stellar Orbits

Scientific paper

New photoelectric observations of the 6th magnitude suspected eclipsing
binary system HD 208496 are presented. A Wilson-Devinney light curve
solution reveals a detached system with components approaching the
terminal age main sequence. The orbital period is suspected to be
variable.

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