SIMBAD references

2002MNRAS.336.1030P - Mon. Not. R. Astron. Soc., 336, 1030-1042 (2002/November-1)

The status of Galactic field λ Bootis stars in the post-Hipparcos era.

PAUNZEN E., ILIEV I.K., KAMP I. and BARZOVA I.S.

Abstract (from CDS):

The λ Bootis stars are Population I, late B- to early F-type stars, with moderate to extreme (up to a factor 100) surface underabundances of most Fe-peak elements and solar abundances of lighter elements (C, N, O and S). To put constraints on the various existing theories that try to explain these peculiar stars, we investigate the observational properties of λ Bootis stars compared with a reference sample of normal stars. Using various photometric systems and Hipparcos data, we analyse the validity of standard photometric calibrations, elemental abundances, and Galactic space motions.

There crystallizes a clear picture of a homogeneous group of Population I objects found at all stages of their main-sequence evolution, with a peak at about 1 Gyr. No correlation of astrophysical parameters such as the projected rotational velocities or elemental abundances with age is found, suggesting that the a priori unknown mechanism, which creates λ Bootis stars, works continuously for late B- to early F-type stars in all stages of main-sequence evolution. Surprisingly, the sodium abundances seem to indicate an interaction between the stars and their local environment.


Abstract Copyright: RAS

Journal keyword(s): stars: chemically peculiar - stars: early-type.

Simbad objects: 124

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2020.01.28-23:30:33

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