Kniha Circularization and Tidal Dissipation in Eclipsing Binary Stars Lorenzo Faccioli

Circularization and Tidal Dissipation in Eclipsing Binary Stars

Results for early type binaries in the Magellanic Clouds from the MACHO project.

Jazyk: Angličtina
Vazba: Brožovaná
Vydavatel: VDM Verlag
Dostupnost: U nakladatele na objednávku
Odesíláme za 17-27 dnů
1 875
This work studies orbital circularization of binary§stars past the Main Sequence using two new sampl...

Informace o knize

Jazyk
Angličtina
Vazba
Kniha - Brožovaná
Vydáno
2008
Stránek
204
EAN
9783639085884
ISBN
3639085884
Enbook ID
06817759
Vydavatel
Hmotnost
281
Rozměry
152 x 229 x 11

Kompletní popis

This work studies orbital circularization of binary§stars past the Main Sequence using two new samples of§eclipsing binary stars found in the Magellanic Clouds§by the MACHO Project, as well as samples introduced§by the OGLE-II project and finds strong evidence of§orbit circularization past the Main Sequence phase of§stellar evolution, by the almost complete absence of§systems with eccentric orbits in the Red Giant part§of the Color Magnitude Diagram whereas the Main§Sequence exhibits systems with a broad range of§eccentricities.§This absence allows to robustly conclude that binary§stars§circularize their orbits either on crossing the§Hertzsprung Gap or on ascending the Red Giant Branch§when they undergo a sudden and dramatic increase in§their dimensions resulting in strong tidal forces§that disrupt the orbit.§The work then quantifies the effects of tidal§interaction and distortions via a a thorough study of§the Specific Dissipation Function Q, which is§generally not well known for binary stars and finds§evidence of a low degree of tidal dissipation.

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