Discovery of magnetic field variations with the 12.1-minute pulsation period of the roAp star γ Equulei

Astronomy and Astrophysics

Volumn 407, Issue 3, 2003, Pages

  Leone, F ^a   Kurtz, D W ^b  

^a INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^b UNIVERSITY OF CENTRAL LANCASHIRE   (United Kingdom)

Author keywords

Stars: chemically peculiar; Stars: individual: HD 201601; Stars: magnetic fields; Stars: oscillations

Indexed keywords

DOPPLER EFFECT; IMAGING TECHNIQUES; MAGNETIC FIELD EFFECTS; PHOTOMETRY;

PULSATION PERIOD;

ASTROPHYSICS;

EID: 0042433138     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031067     Document Type: Article

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