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Formation of resonance spectral line profiles in stellar wind: Theory and observations
DOI: 10.1080/10556799908203004 Bibcode: 1999A&AT...18..475S

Sapar, L.; Sapar, A.

The theory of the formation of resonance spectral line profiles in the stellar wind of hot stars has been elaborated taking into account the presence of microturbulent motions. In this case the local frequency redistribution in the line profile function is incomplete. This circumstance generates dominating backscattering of photons and drastic cha…

1999 Astronomical and Astrophysical Transactions
IUE 3
New Insights on Late-A and Early-F Star Activity
DOI: 10.1080/10556799708213569 Bibcode: 1997A&AT...14...41F

Talavera, A.; Freire Ferrero, R.; Bruhweiler, F. +3 more

The onset of chromospheric activity in late-A and early-F stars is here discussed. The detection of Ly- emission core in several A and F atars with the IUE satellite, gives evidence for the presence of chromospheric layers in these stars up to B - V = 0m.19 (Marilli et al., 1996). Semiempirical chromospheric models for Altair allowed us (Freire Fe…

1997 Astronomical and Astrophysical Transactions
IUE 0