Particle Transport in Non-Magnetic Stars
1986 ◽
Vol 90
◽
pp. 459-472
Keyword(s):
AbstractThe observations of AmFm, λ Booti, HgMn and He rich stars that are explained without any arbitrary parameter by diffusion are briefly reviewed, followed by those observations that are not explained by this simple model. Mass loss is then shown to explain a large fraction of the observations that are not explained in the parameter free model. It seems to play a role in the λ Booti, AmFm, He rich and the hot horizontal branch stars. It is only of about 10−15 to 10−13 Mo/yr. Abundance anomalies then help to determine stellar hydrodynamics. It is finally suggested that recent observations of Li underabundances in F stars of the Hyades represent an extension of the AmFm star phenomenon.
1991 ◽
Vol 145
◽
pp. 111-124
Keyword(s):
1997 ◽
Vol 189
◽
pp. 363-368
Keyword(s):
On the Interpretation of RR Lyrae Properties in Globular Clusters and in Other Population II Systems
1973 ◽
Vol 21
◽
pp. 197-206
Keyword(s):
1985 ◽
Vol 87
◽
pp. 453-469
Keyword(s):
2002 ◽
Vol 392
(2)
◽
pp. 553-562
◽
2019 ◽
Vol 14
(S351)
◽
pp. 341-345