Multisite observations of SU aurigae

Monthly Notices of the Royal Astronomical Society

Volumn 348, Issue 4, 2004, Pages 1301-1320

  Unruh, Y C ^a   Donati, J F ^b   Oliveira, J M ^c,d   Cameron, A Collier ^e   Catala, C ^b   Henrichs, H F ^f   Johns Krull, C M ^g   Foing, B ^c   Hao, J ^h   Cao, H ^h   Landstreet, J D ⁱ   Stempels, H C ^j   De Jong, J A ^k   Telting, J ^l   Walton, N ^m   Ehrenfreund, P ^k   Hatzes, A P ^n,o   Neff, J E ^p   Bohm T ^b   Simon, T ^q   Kaper, L ^f   Strassmeier, K G ^r   Granzer, Th ^r   more..

^a IMPERIAL COLLEGE LONDON   (United Kingdom)

^b IRAP   (France)

^c EUROPEAN SPACE AGENCY   (Netherlands)

^d KEELE UNIVERSITY   (United Kingdom)

^e UNIVERSITY OF ST ANDREWS   (United Kingdom)

^f UNIVERSITY OF AMSTERDAM   (Netherlands)

^g RICE UNIVERSITY   (United States)

^h CHINESE ACADEMY OF SCIENCES   (China)

ⁱ UNIVERSITY OF WESTERN ONTARIO   (Canada)

^j Box 515   (Sweden)

^k LEIDEN UNIVERSITY   (Netherlands)

^l NORDIC OPTICAL TELESCOPE   (Spain)

^m UNIVERSITY OF CAMBRIDGE   (United Kingdom)

ⁿ The University of Texas at Austin   (United States)

^o THÜRINGER LANDESSTERNWARTE TAUTENBURG   (Germany)

^p School of Business   (United States)

^q UNIVERSITY OF HAWAII   (United States)

^r ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

more..

Author keywords

Stars: imaging; Stars: individual: SU Aur; Stars: magnetic fields; Stars: pre main sequence

Indexed keywords

MAGNETIC FIELDS; STARS;

BALMER LINES; D-PERIODICITY; MULTI-SITE; MULTISITE OBSERVATIONS; OUT OF PHASE; STARS: INDIVIDUAL: SU AUR; STARS: MAGNETIC FIELD; STARS: PRE-MAIN SEQUENCE; STARS:IMAGING; T TAURI STARS;

SIGNAL TO NOISE RATIO;

EID: 1642390685     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07445.x     Document Type: Review

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