In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2
G.m. Wahlgren
Detaily:
Rok, strany: 2008, 279 - 284
Kľúčové slová:
stars: B-type, stars: chemically peculiar, spectral lines: emission
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2008/Vol_38/No_2/pp279-284_abstract.html
O článku:
Weak emission lines (WELs) of metals are observed in sharp-lined spectra of
mid- to late-B type stars. The WELs are detected over a range of element
abundance and are found among both chemically-normal and chemically-peculiar
stars. The characteristics of this ubiquitous phenomenon are reviewed and their
potential for the study of inhomogeneous stellar atmospheres is presented.
Ako citovať:
ISO 690:
Wahlgren, G. 2008. Weak emission lines and peculiar stars. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no.2, pp. 279-284. 1335-1842.
APA:
Wahlgren, G. (2008). Weak emission lines and peculiar stars. Contributions of the Astronomical Observatory Skalnaté Pleso, 38(2), 279-284. 1335-1842.