Tallenna
Hydrogen Deficient Stars and Related Objects
The first helium star was discovered in 1942, the first scientific meeting on the subject, however, took place in 1985. It becomes less manifest in cool stars, where the temperature is too low to excite helium and where one has to devise indirect methods for proving hydrogen deficiency.
- Alaotsikko
- Proceeding of the 87th Colloquium of the International Astronomical Union Held at Mysore, India, 10–15 Nevember 1985
- Toimittaja
- K. Hunger, Detlef Schönberner, N.K. Rao
- Painos
- Softcover reprint of the original 1st ed. 1986
- ISBN
- 9789401086080
- Kieli
- englanti
- Paino
- 310 grammaa
- Julkaisupäivä
- 13.10.2011
- Kustantaja
- Springer
- Sivumäärä
- 528
