Magnetic fields in intermediate- and high-mass binary systems with short periods

Nazé, Yaël; Alecian, E.

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Magnetic fields in intermediate- and high-mass binary systems with short periods

Nazé, Yaël; Alecian, E.

2018 • In Contributions of the Astronomical Observatory Skalnaté Pleso, 48, p. 98-105

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Keywords :

stars: magnetic field; stars: massive; binaries: general

Abstract :

[en] Most stars of the upper HRD live in multiple systems. When the separation is small, interactions may occur, affecting the stellar evolution and feedback. The presence of magnetic fields here opens the door to phenomena beyond the "usual" ones (mass transfer, wind collisions, tidal interactions,...) but it also put strong constraints on models of stellar evolution and magnetic field generation. This is why surveys of intermediate- and high-mass binaries with short periods have been undertaken. We will review results in this domain, including the properties of the (rare) detected cases such as Plaskett's star.

Disciplines :

Space science, astronomy & astrophysics

Author, co-author :

Nazé, Yaël ; Université de Liège - ULiège > Groupe d'astrophysique des hautes énergies (GAPHE)

Alecian, E.

Language :

English

Title :

Magnetic fields in intermediate- and high-mass binary systems with short periods

Publication date :

01 January 2018

Journal title :

Contributions of the Astronomical Observatory Skalnaté Pleso

ISSN :

1335-1842

eISSN :

1336-0337

Publisher :

Slovak Academy of Sciences. Astronomical Institute, Tatranská Lomnica, Slovakia

Volume :

Pages :

98-105

Peer reviewed :

Peer Reviewed verified by ORBi

Additional URL :

http://cdsads.u-strasbg.fr/abs/2018CoSka..48...98N

Available on ORBi :

since 06 March 2018

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