Photometric Study of HD224085

Details Photometric Study of HD224085 Photometric Study of HD224085

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.196..289r&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 196, P. 289, 1981

Astronomy and Astrophysics

Astronomy

21

Scientific paper

B and V photometry of HD 224085 obtained on 21 nights between 1979 November and 1980 February is presented. The amplitudes of light variation observed are ˜0.15 mag in both B and V. The photometric period is found to be Pphot = 6.7026l±0.0034 day. A new orbital solution obtained from the available radial velocity data shows that the orbital period is 6.724464 day. The radius of the visible primary estimated from the Barnes-Evans surface brightness relation is ˜1.9 Rsun., indicating a position above the main sequence.

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