In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2
P.l. North - J. Babel - D. Erspamer
Details:
Year, pages: 2008, 375 - 384
Keywords:
stars: chemically peculiar, stars: magnetic fields, stars: evolution, stars: rotation, stars: statistics
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2008/Vol_38/No_2/pp375-384_abstract.html
About article:
The many peculiarities of Ap stars (not only chemical ones, but also
magnetic field and slow rotation) may vary during the main-sequence evolution
of these stars. We review here briefly the evidences found in the last thirty
years for such evolution, with an emphasis on the more recent research. The
position in the HR diagram of low mass Ap stars with a significant surface
magnetic field (as measured by us) is reviewed as well.
How to cite:
ISO 690:
North, P., Babel, J., Erspamer, D. 2008. The evolution of Ap stars. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no.2, pp. 375-384. 1335-1842.
APA:
North, P., Babel, J., Erspamer, D. (2008). The evolution of Ap stars. Contributions of the Astronomical Observatory Skalnaté Pleso, 38(2), 375-384. 1335-1842.