The young close binary HD 47732 in NGC 2264

Details The young close binary HD 47732 in NGC 2264 The young close binary HD 47732 in NGC 2264

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...222..574k&link_type=abstract

Astrophysical Journal, Part 1, vol. 222, June 1, 1978, p. 574-577.

Astronomy and Astrophysics

Astrophysics

8

Binary Stars, Star Clusters, Stellar Spectra, Variable Stars, Light Curve, Stellar Spectrophotometry

Scientific paper

HD 47732 is a short-period, ellipsoidal variable with some complications evident in its yellow light curve. The interpretation of the light curve is entirely dependent upon spectroscopic information. The seeming best spectral classifications lead to a contact configuration. Spectral types that are only slightly later lead to a semidetached description. Either interpretation of HD 47732 implies a distance of at least 1.2 kpc, considerably greater than the commonly accepted distance for the cluster NGC 2264 of which it is a member.

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