In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2
M. Thiam - G.a. Wade - F. Leblanc - V.r. Khalack
Details:
Year, pages: 2008, 461 - 462
Keywords:
stars: chemically peculiar, stars: abundances
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2008/Vol_38/No_2/pp461-462_abstract.html
About article:
Photospheric abundance determinations for several HgMn stars were undertaken
using archival ESO-UVES spectra.
Unblended lines in the visible region of the spectrum of the elements Ti, Cr,
Mn and Fe were used
to obtain their abundance and to search for the presence of abundance
stratification as a function of optical depth. Results are reported for
HD 178065 and HD 175640. Of the elements studied, only Mn shows
signs of abundance stratification.
How to cite:
ISO 690:
Thiam, M., Wade, G., Leblanc, F., Khalack, V. 2008. Search for abundance stratification in the atmospheres of HgMn stars. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no.2, pp. 461-462. 1335-1842.
APA:
Thiam, M., Wade, G., Leblanc, F., Khalack, V. (2008). Search for abundance stratification in the atmospheres of HgMn stars. Contributions of the Astronomical Observatory Skalnaté Pleso, 38(2), 461-462. 1335-1842.