Multi-element abundance Doppler imaging of the rapidly oscillating Ap star HR 3831

Astronomy and Astrophysics

Volumn 424, Issue 3, 2004, Pages 935-950

  Kochukhov, O ^a   Drake, N A ^b,c   Piskunov, N ^d   De La Reza, R ^b  

^a UNIVERSITY OF VIENNA   (Austria)

^b OBSERVATÓRIO NACIONAL   (Brazil)

^c ST PETERSBURG STATE UNIVERSITY   (Russian Federation)

^d UPPSALA UNIVERSITY   (Sweden)

Author keywords

Stars: chemically peculiar; Stars: individual: HR 3831; Stars: magnetic fields

Indexed keywords

ASTROPHYSICS; DIFFUSION; DOPPLER EFFECT; ESTIMATION; MAGNETIC FIELD EFFECTS; OPTICAL RESOLVING POWER; ROTATION; SPECTRUM ANALYSIS; SURFACE STRUCTURE; TOPOLOGY;

STARS: CHEMICALLY PECULIAR; STARS: INDIVIDUAL: HR 3831; STARS: MAGNETIC FIELDS;

IMAGING TECHNIQUES;

EID: 4644313720     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040517     Document Type: Article

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