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- W1994886621 abstract "We report photometric observations, an analysis of the resulting light curve, and a preliminary model for the eclipsing binary V1147 Cygni (GSC 2660-2608; ). V1147 Cyg is a detached eclipsing m p 12.0 V system of A-type stars. The sidereal period of the system is 15.2513228(7) days, with an eccentric orbit of e p 0.275(12) and evidence of apsidal motion on the order of 0 .80(11) per century. Our analysis indicates that the stars are well separated and should yield precise main-sequence dimensions. Thus, this is a valuable system in several respects. Online material: extended table" @default.
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- W1994886621 date "2006-03-01" @default.
- W1994886621 modified "2023-10-14" @default.
- W1994886621 title "Photometric Study of the Eccentric‐Orbit Binary V1147 Cygni" @default.
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- W1994886621 doi "https://doi.org/10.1086/499630" @default.
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