Line profile variations in rapidly oscillating Ap stars: Resolution of the enigma

Monthly Notices of the Royal Astronomical Society

Volumn 376, Issue 2, 2007, Pages 651-672

  Kochukhov, O ^a   Ryabchikova, T ^b,c   Weiss, W W ^c   Landstreet, J D ^d   Lyashko, D ^e  

^a UPPSALA UNIVERSITY   (Sweden)

^b INSTITUTE OF ASTRONOMY   (Russian Federation)

^c UNIVERSITY OF VIENNA   (Austria)

^d UNIVERSITY OF WESTERN ONTARIO   (Canada)

^e TAURIDA NATIONAL V I VERNADSKY UNIVERSITY   (Ukraine)

Author keywords

Line: profiles; Stars: chemically peculiar; Stars: magnetic field; Stars: oscillations

Indexed keywords

LINEWIDTH; METAL IONS; NEODYMIUM COMPOUNDS; PRASEODYMIUM COMPOUNDS; RARE EARTHS; STARS; TELESCOPES; VELOCITY;

HIGH RESOLUTION; HIGH SIGNAL-TO-NOISE RATIO; LINE: PROFILES; STAR OSCILLATIONS; STARS: CHEMICALLY PECULIAR; STARS: MAGNETIC FIELD; STELLARS; TIMES SERIES; VARIABILITY PATTERNS; VERY LARGE TELESCOPE;

SIGNAL TO NOISE RATIO;

EID: 34247199576     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.11449.x     Document Type: Article

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