Further confirmations of mass transfer in Algol type binary U Sagittae

Details Further confirmations of mass transfer in Algol type binary U Sagittae Further confirmations of mass transfer in Algol type binary U Sagittae

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ap%26ss.313..339m&link_type=abstract

Astrophysics and Space Science, Volume 313, Issue 4, pp.339-344

Astronomy and Astrophysics

Astrophysics

2

Stars, Binaries, Eclipsing, Stars, Mass Transfer, Stars&Rsquo, Magnetic Fields, Stars-Individuals, U Sge

Scientific paper

This paper describes how a new photometric V light curve solution of Algol type binary U Sge was obtained using Wilson Devinney code. I also discuss how the physical and orbital parameters, along with absolute dimensions of the system, were determined. The Roche lobe configurations of the system indicate that the secondary component has filled its Roche lobe and therefore is losing mass at the rate of 6.15×10-7 M sun yr-1. The conservative mass flow is the most likely process in this system.

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