Tallenna
Pulsation, Rotation and Mass Loss in Early-Type Stars
In this Symposium, researchers specializing in pulsation, rotation, magnetic fields and stellar winds are brought together for the first time in order to broaden our understanding of O and B stars. The variability of radiatively-driven winds from O and B stars are likely related to the rotation of the star.
- Alaotsikko
- Proceedings of the 162nd Symposium of the International Astronomical Union, Held in Antibes-Juan-Les-Pins, France, October 5–8, 1993
- Toimittaja
- Luis A. Balona, Huib F. Henrichs, Jean Michel Le Contel
- Painos
- Softcover reprint of the original 1st ed. 1994
- ISBN
- 9780792330455
- Kieli
- englanti
- Paino
- 310 grammaa
- Julkaisupäivä
- 31.8.1994
- Kustantaja
- Springer
- Sivumäärä
- 550
