The Lorentz force in atmospheres of chemically peculiar stars: 56 Arietis

Astronomy and Astrophysics

Volumn 509, Issue 1, 2010, Pages

  Shulyak, D ^a   Kochukhov, O ^b   Valyavin, G ^c   Lee, B C ^d   Galazutdinov, G ^e   Kim, K M ^d   Han, I ^d   Burlakova, T ^f  

^a UNIVERSITY OF VIENNA   (Austria)

^b UPPSALA UNIVERSITY   (Sweden)

^c UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^d Korea Astronomy and Space Science Institute (KASI)   (South Korea)

^e Seoul National University   (South Korea)

^f RUSSIAN ACADEMY OF SCIENCES   (Russian Federation)

Author keywords

56 Ari Stars; Atmospheres; Chemically peculiar Stars; Individual; Magnetic field Stars; Stars

Indexed keywords

ATMOSPHERIC STRUCTURE; ELECTRIC CURRENT MEASUREMENT; ELECTRIC POWER SUPPLIES TO APPARATUS; LORENTZ FORCE; MAGNETIC FIELD EFFECTS; MAGNETIC MATERIALS; MAGNETISM; PRESSURE EFFECTS; SPECTROSCOPY;

ATMOSPHERES; BALMER LINES; CHEMICALLY PECULIAR; CHEMICALLY PECULIAR-STARS; HIGH-RESOLUTION SPECTROSCOPIC OBSERVATIONS; HYDROGEN LINES; MAGNETIC PRESSURE; MODEL ATMOSPHERE; PLASMA PROPERTIES; PRESSURE SENSITIVE; QUADRUPOLE CONFIGURATION; ROTATION CYCLE; SPECTRAL LINE; SPECTROSCOPIC FEATURES; STARS - STARS; STARS ATMOSPHERES; STELLAR MODEL ATMOSPHERES;

STARS;

EID: 76349084287     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912615     Document Type: Article

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