In between β Lyrae and Algol: The Case Of V356 Sgr

The eclipsing binary system V356 Sgr is of considerable interest, since it is probably at the very end of its mass transfer phase, i.e. between beta Lyrae and Algol. Hence, the binary provides an opportunity to directly examine the exposed core of a star for signatures of nuclear burning, and to tes...

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Veröffentlicht in:	Astrophysics and space science 2005-01, Vol.296 (1-4), p.189-192
Hauptverfasser:	Dominis, D., Mimica, P., Pavlovski, K., TAMAJO, E.
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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