In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2
D. Shulyak - O. Kochukhov - S. Khan
Detaily:
Rok, strany: 2008, 449 - 450
Kľúčové slová:
stars: chemically peculiar, stars: magnetic fields, stars: atmospheres
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2008/Vol_38/No_2/pp449-450_abstract.html
O článku:
We present the results of modeling the atmosphere of one of the
extreme magnetic CP star HD 137509, which has the mean surface
magnetic field module of about 29 kG. Such a strong field,
as well as clearly observed abundance peculiarities, make this star
one of the most preferable target for testing our assumptions about
the atmospheric structure of magnetic stars. The calculations presented
are based on resent version of the LLMODELS stellar model atmosphere code
which accounts for full treatment of Zeeman splitting of spectral
lines and polarized radiative transfer.
Ako citovať:
ISO 690:
Shulyak, D., Kochukhov, O., Khan, S. 2008. Model atmospheres of magnetic CP stars: HD 137509. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no.2, pp. 449-450. 1335-1842.
APA:
Shulyak, D., Kochukhov, O., Khan, S. (2008). Model atmospheres of magnetic CP stars: HD 137509. Contributions of the Astronomical Observatory Skalnaté Pleso, 38(2), 449-450. 1335-1842.