In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2
Iliev.i.kh. - J. Budaj
Details:
Year, pages: 2008, 129 - 134
Keywords:
stars: chemically peculiar, stars: binaries: general, stars: abundances
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2008/Vol_38/No_2/pp129-134_abstract.html
About article:
It is argued that apart from the well known dependence of
the Am phenomenon on mass, age (effective temperature, gravity)
and rotation there is also a complex dependence on the orbital
parameters in binary systems.
This is why the generally accepted scenario in which
the Am star's rotation plays a unique role needs to be revisited,
the strong correlations between the rotation,
orbital period and eccentricity need to be properly
addressed, and tidal effects should be taken into account.
Recent observations of Am stars in binary systems are reviewed.
How to cite:
ISO 690:
Iliev.i.kh., ., Budaj, J. 2008. Am stars in binary systems. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no.2, pp. 129-134. 1335-1842.
APA:
Iliev.i.kh., ., Budaj, J. (2008). Am stars in binary systems. Contributions of the Astronomical Observatory Skalnaté Pleso, 38(2), 129-134. 1335-1842.