The EUV Source HD 52452: Discovery of a Likely Triple System

Details The EUV Source HD 52452: Discovery of a Likely Triple System The EUV Source HD 52452: Discovery of a Likely Triple System

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ibvs.5014....1m&link_type=abstract

Information Bulletin on Variable Stars, 5014, 1.

Computer Science

1

Photometry And Spectroscopy

Scientific paper

We present the results of a photometric and spectroscopic study of the
EUV bright source HD 52452. This star results to be a triple system
composed by a SB1 G5:V+G5:V close binary, which rotates with a period
P=0.423 days and by a slower rotating G5:V companion.

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