Inhomogeneous surface distribution of chemical elements in the eclipsing binary AR Aur: A new challenge for our understanding of HgMn stars

Monthly Notices of the Royal Astronomical Society

Volumn 371, Issue 4, 2006, Pages 1953-1958

  Hubrig, S ^a   Gonzalez J F ^b   Savanov, I ^c   Scholler M ^a   Ageorges, N ^a   Cowley, C R ^d   Wolff, B ^e  

^a EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^b Complejo Astronómico El Leoncito ^*  (Argentina)

^c ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^d UNIVERSITY OF MICHIGAN   (United States)

^e EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

Binaries: eclipsing; Binaries: spectroscopic; Stars: abundances; Stars: chemically peculiar; Stars: individual: AR Aur; Stars: individual: And

Indexed keywords

CADMIUM ALLOYS; HELIUM; MANGANESE ALLOYS; MERCURY AMALGAMS; SPECTRAL RESOLUTION; STARS;

BINARIES: SPECTROSCOPIC; BINARIES:ECLIPSING; ECLIPSING BINARIES; PRIMARY STARS; STAR: INDIVIDUAL: AR AUR; STAR: INDIVIDUAL:Α AND; STARS ABUNDANCES; STARS: CHEMICALLY PECULIAR; STARS: INDIVIDUAL: PROXIMA CENTAURI;

BINARY ALLOYS;

EID: 33748676455     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10863.x     Document Type: Article

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