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A&A manuscript no. (will be inserted by hand later)
 

Summary: A&A manuscript no.
(will be inserted by hand later)
Your thesaurus codes are:
02(02.13.1; 02.16.2; 08.03.2)
ASTRONOMY
AND
ASTROPHYSICS
5.2.1996
Multipolar magnetic fields in rotating Ap stars:
modeling of observable quantities
S. Bagnulo 1 , M. Landi Degl'Innocenti 2 , and E. Landi Degl'Innocenti 3
1 Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland
2 C.N.R., Gruppo Nazionale di Astronomia, Unit`a di Ricerca di Arcetri, Largo E. Fermi 5, I­50125 Firenze, Italy
3 Dipartimento di Astronomia e Scienza dello Spazio, Universit`a di Firenze, Largo E. Fermi 5, I­50125 Firenze, Italy
Received 11 May, accepted 28 August 1995
Abstract. Magnetic field is present in most of the chem­
ically peculiar stars of the upper main sequence. For a
long time, the component of the magnetic field along the
line of sight and the magnetic field modulus, averaged on
the stellar disk, were the only diagnostic contents of the

  

Source: Armagh Observatory

 

Collections: Physics