A photometric study of the recently discovered eclipsing binary V776 Cassiopei

New Astronomy

Volumn 9, Issue 6, 2004, Pages 425-434

  Djurasevic G ^a,b   Albayrak, B ^c   Selam, S O ^c   Erkapic S ^a,b   Senavci H V ^c  

^a ASTRONOMICAL OBSERVATORY   (Serbia)

^b ISAAC NEWTON INSTITUTE OF CHILE   (Chile)

^c ANKARA UNIVERSITY   (Turkey)

Author keywords

Binaries: close; Binaries: eclipsing; Stars: fundamental parameters; Stars: individual: V776 Cas

Indexed keywords

COMPUTER SIMULATION; ENERGY TRANSFER; GALAXIES; LIGHT PROPAGATION; MASS TRANSFER; PARAMETER ESTIMATION; PHOTOELECTRICITY; PHOTOMETRY;

CLOSE BINARIES; ECLIPSING BINARIES; STARS; STARS: V776 CASSIPEI;

ASTRONOMY;

EID: 1842843038     PISSN: 13841076     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.newast.2004.02.001     Document Type: Article

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