SIMBAD references

2008A&A...481..453M - Astronomy and Astrophysics, volume 481, 453-463 (2008/4-2)

Nitrogen enrichment, boron depletion and magnetic fields in slowly-rotating B-type dwarfs.

MOREL T., HUBRIG S. and BRIQUET M.

Abstract (from CDS):

Evolutionary models for massive stars, accounting for rotational mixing effects, do not predict any core-processed material at the surface of B dwarfs with low rotational velocities. Contrary to theoretical expectations, we present a detailed and fully-homogeneous, NLTE abundance analysis of 20 early B-type dwarfs and (sub)giants that reveals the existence of a population of nitrogen-rich and boron-depleted, yet intrinsically slowly-rotating objects. The low-rotation rate of several of these stars is firmly established, either from the occurrence of phase-locked UV wind line-profile variations, which can be ascribed to rotational modulation, or from theoretical modelling in the pulsating variables. The observational data presently available suggest a higher incidence of chemical peculiarities in stars with a (weak) detected magnetic field. This opens the possibility that magnetic phenomena are important in altering the photospheric abundances of early B dwarfs, even for surface field strengths at the one hundred Gauss level. However, further spectropolarimetric observations are needed to assess the validity of this hypothesis.

Abstract Copyright:

Journal keyword(s): stars: early-type - stars: fundamental parameters - stars: abundances - stars: atmospheres - stars: magnetic fields

Simbad objects: 29

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2019.09.15-16:49:10

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