Add to ORKGA small fraction of intermediate-mass main sequence (A and B type) stars have strong, organised magnetic fields. The large majority of such stars, however, show no evidence for magnetic fields, even when observed with very high precision. In this paper we describe a simple model, motivated by qualitatively new observational results, that provides a natural physical explanation for the small fraction of observed magnetic stars
To date, only a small number of O and early B-type stars have been investigated for magnetic fields,...
Aims.We investigated a sample of 28 well-known spectroscopically-identified magnetic Ap/Bp stars, wi...
International audienceContext : .The origin of the fossil magnetic fields detected in 5 to 10% of in...
A small fraction of intermediate-mass main sequence (A and B type) stars have strong, organised magn...
Context.About 5% of upper main sequence stars are permeated by a strong magnetic field, the origin o...
Accepted by Astronomy & Astrophysics, 17 Sept. 07. 23 pages, 32 figuresInternational audienceWe have...
Magnetic fields have been detected on stars across the H-R diagram and substellar objects ...
We consider the incidence of magnetism in main-sequence stars with mainly radiative envelopes. We pr...
The dates of receipt and acceptance should be inserted later We present the result of a highly sensi...
Magnetic fields play an important role in producing and modifying the photospheric chemical peculiar...
About 5% of upper main sequence stars are permeated by a strong magnetic field, the origin of which ...
This paper first surveys how stellar magnetic fields are measured, and especially the impact of the ...
École Evry Schatzman de Physique Stellaire du PNPS XXIIIInternational audienceMagnetic fields have b...
Aims. We investigated a sample of 28 well-known spectroscopically-identified magnetic Ap/Bp stars, w...
This review presents a general overview of the magnetic fields found in main sequence A and B stars,...
To date, only a small number of O and early B-type stars have been investigated for magnetic fields,...
Aims.We investigated a sample of 28 well-known spectroscopically-identified magnetic Ap/Bp stars, wi...
International audienceContext : .The origin of the fossil magnetic fields detected in 5 to 10% of in...
A small fraction of intermediate-mass main sequence (A and B type) stars have strong, organised magn...
Context.About 5% of upper main sequence stars are permeated by a strong magnetic field, the origin o...
Accepted by Astronomy & Astrophysics, 17 Sept. 07. 23 pages, 32 figuresInternational audienceWe have...
Magnetic fields have been detected on stars across the H-R diagram and substellar objects ...
We consider the incidence of magnetism in main-sequence stars with mainly radiative envelopes. We pr...
The dates of receipt and acceptance should be inserted later We present the result of a highly sensi...
Magnetic fields play an important role in producing and modifying the photospheric chemical peculiar...
About 5% of upper main sequence stars are permeated by a strong magnetic field, the origin of which ...
This paper first surveys how stellar magnetic fields are measured, and especially the impact of the ...
École Evry Schatzman de Physique Stellaire du PNPS XXIIIInternational audienceMagnetic fields have b...
Aims. We investigated a sample of 28 well-known spectroscopically-identified magnetic Ap/Bp stars, w...
This review presents a general overview of the magnetic fields found in main sequence A and B stars,...
To date, only a small number of O and early B-type stars have been investigated for magnetic fields,...
Aims.We investigated a sample of 28 well-known spectroscopically-identified magnetic Ap/Bp stars, wi...
International audienceContext : .The origin of the fossil magnetic fields detected in 5 to 10% of in...