[HTML][HTML] The relation between rotational velocities and spectral peculiarities among A-type stars
HA Abt, NI Morrell - Astrophysical Journal Supplement v. 99, p …, 1995 - adsabs.harvard.edu
The Relation between Rotational Velocities and Spectral Peculiarities among A-Ty ADS Classic
is now deprecated. It will be completely retired in October 2019. This page will automatically …
is now deprecated. It will be completely retired in October 2019. This page will automatically …
The lithium abundance in stars
G Michaud, P Charbonneau - Space Science Reviews, 1991 - Springer
The observations of Li abundances in pre-Main-Sequence, Main-Séquence (Population I
and II), sub-giant, and giant stars are reviewed in order to show how Li can be used as a …
and II), sub-giant, and giant stars are reviewed in order to show how Li can be used as a …
The evolution of AmFm stars, abundance anomalies, and turbulent transport
Stellar evolution models of stars of 1.45–3.0 M⊙ have been calculated, including the atomic
diffusion of metals and radiative accelerations for all species in the OPAL opacities. As the …
diffusion of metals and radiative accelerations for all species in the OPAL opacities. As the …
The VAST Survey–III. The multiplicity of A-type stars within 75 pc
With a combination of adaptive optics imaging and a multi-epoch common proper motion
search, we have conducted a large volume-limited (D≤ 75 pc) multiplicity survey of A-type …
search, we have conducted a large volume-limited (D≤ 75 pc) multiplicity survey of A-type …
[BOOK][B] Atomic diffusion in stars
G Michaud, G Alecian, J Richer - 2015 - Springer
Atomic diffusion is a fundamental physical process. Its universal presence is not questioned.
Yet, in stellar astrophysics it is often abusively ignored. Arguments that it plays a negligible …
Yet, in stellar astrophysics it is often abusively ignored. Arguments that it plays a negligible …
The δ Scuti stars of the Cep–Her Complex – I. Pulsator fraction, rotation, asteroseismic large spacings, and the νmax relation
ABSTRACT We identify delta Scuti (Sct) pulsators amongst members of the recently
discovered Cep–Her Complex using light curves from the Transiting Exoplanet Survey …
discovered Cep–Her Complex using light curves from the Transiting Exoplanet Survey …
Simulations of core convection in rotating A-type stars: differential rotation and overshooting
We present the results of three-dimensional simulations of core convection within A-type
stars of 2 M☉, at a range of rotation rates. We consider the inner 30% by radius of such …
stars of 2 M☉, at a range of rotation rates. We consider the inner 30% by radius of such …
[BOOK][B] Magnetic fields in O, B, and A stars
S Hubrig, M Schöller - 2021 - iopscience.iop.org
The last few decades have seen significant progress in our understanding of the occurrence
of magnetic fields in stars with radiative envelopes, in particular in massive stars and in …
of magnetic fields in stars with radiative envelopes, in particular in massive stars and in …
[HTML][HTML] The lithium abundance gap in the Hyades F stars-The signature of diffusion
G Michaud - Astrophysical Journal, Part 1 (ISSN 0004-637X) …, 1986 - adsabs.harvard.edu
The lithium abundance gap in the Hyades F stars - The signature of diffusion ADS Classic is now
deprecated. It will be completely retired in October 2019. This page will automatically redirect to …
deprecated. It will be completely retired in October 2019. This page will automatically redirect to …
Consistent evolution of F stars: diffusion, radiative accelerations, and abundance anomalies
Consistent stellar evolution models of F stars (1.1–1.5 M &sun;) are calculated with radiative
forces, opacities, and diffusion for all elements included in OPAL's opacity tables. The …
forces, opacities, and diffusion for all elements included in OPAL's opacity tables. The …