Interacting Binary Star Environments and the W Ser - DPV - Algol Connection

dc.creatorMennickent, R. E.
dc.creatorKolaczkowski, Z.
dc.date2009-04-09
dc.date.accessioned2026-07-07T13:01:58Z
dc.date.available2026-07-07T13:01:58Z
dc.descriptionRecent work on some kinds of interacting binaries is summarized, with emphasis on Cataclysmic Variables, Algol-like variables and the recently discovered Double Periodic Variables (DPVs). The sequence W Serpentids (very massive with irregular variability and large mass loss) $\to$ DPVs (less massive with regular variability and ciclic mass loss) $\to$ Algols (even less massive with small mass loss) could correspond to an evolutionary sequence, and illustrate the importance of the mass transfer rate in shaping observable and mass loss properties for these systems.
dc.descriptionInvited talk to the ESO workshop "The Interferometric view on Hot Stars", March 2-6, 2009, Vina del Mar, Chile, to be published in Revista Mexicana de Astronomia y Astrofisica
dc.identifierhttps://arxiv.org/abs/0904.1539
dc.identifierhttp://arxiv.org/abs/0904.1539
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/226331
dc.subjectSolar and Stellar Astrophysics
dc.titleInteracting Binary Star Environments and the W Ser - DPV - Algol Connection
dc.typetext

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