Tallenna
The Symbiotic Phenomenon
Symbiotic stars were identified spectroscopically as M giants with a very strong He II 4686 emission line. We now speak confidently of a "symbiotic phenomenon" , in which an evolved red giant and a hot companion object (usually thought to be an accreting main sequence star or a luminous white dwarf star) happily coexist.
- Alaotsikko
- Proceedings of the 103rd Colloquium of the International Astronomical Union, Held in Torun, Poland, August 18–20, 1987
- Toimittaja
- Joanna Mikolajewska, M. Friedjung, Scott J. Kenyon, Roberto Viotti
- Painos
- Softcover reprint of the original 1st ed. 1988
- ISBN
- 9789401078337
- Kieli
- englanti
- Paino
- 310 grammaa
- Julkaisupäivä
- 9.11.2011
- Kustantaja
- Springer
- Sivumäärä
- 380
