In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2
S. Hubrig - J.f. González - R. Arlt
Detaily:
Rok, strany: 2008, 415 - 416
Kľúčové slová:
stars: abundances, stars: chemically peculiar, stars: magnetic fields, stars: differential rotation
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2008/Vol_38/No_2/pp415-416_abstract.html
O článku:
The important result achieved in our recent study of a large sample of HgMn
stars using UVES at the VLT and FEROS at the ESO 2.2 m telescope is the
finding that most HgMn stars exhibit spectral variability of various
chemical elements, proving that the presence of an inhomogeneous
distribution on the surface of these stars is a rather common characteristic
and not a rare phenomenon.
Ako citovať:
ISO 690:
Hubrig, S., González, J., Arlt, R. 2008. Spots on the surface of HgMn stars: clues to the origin of Hg and Mn peculiarities. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no.2, pp. 415-416. 1335-1842.
APA:
Hubrig, S., González, J., Arlt, R. (2008). Spots on the surface of HgMn stars: clues to the origin of Hg and Mn peculiarities. Contributions of the Astronomical Observatory Skalnaté Pleso, 38(2), 415-416. 1335-1842.