Elemental Abundance Studies of CP Stars the HGMN Group

Details Elemental Abundance Studies of CP Stars the HGMN Group Elemental Abundance Studies of CP Stars the HGMN Group

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006rmxac..26r.182l&link_type=abstract

XI IAU Regional Latin American Meeting of Astronomy (Eds. L. Infante & M. Rubio) Revista Mexicana de Astronomía y Astrofísica (S

Astronomy and Astrophysics

Astronomy

Scientific paper

An analysis of the abundances of the normal late-B star HD 196426 and of the HgMn CP star HD 144206 is presented using ATLAS9 model atmospheres and observational material taken with the SARG spectrograph attached to the Telescopio Nazionale Galileo, Roque de los Muchachos, La Palma, Spain. The isotopic and hyperfine structure of several lines of MnII, GaII, PtII, HgI and HgII in HD 144206 is investigated and also, the possible existence of weak emission lines from CrII and TiII in the red part of the spectrum.

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