
handle: 2268/76354
Main difficulties and uncertainties in stellar physics originate in the modelling of convection, microscopic and macroscopic transport mechanisms and rotation. I consider each of these physical aspects, with a particular attention to their possible probe by asteroseismology. Another important question about opacities is considered by Montalban & Miglio (2008).
Aérospatiale, astronomie & astrophysique, Physical, chemical, mathematical & earth Sciences, Physique, chimie, mathématiques & sciences de la terre, Space science, astronomy & astrophysics
Aérospatiale, astronomie & astrophysique, Physical, chemical, mathematical & earth Sciences, Physique, chimie, mathématiques & sciences de la terre, Space science, astronomy & astrophysics
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 0 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
