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The Symbiotic Phenomenon
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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.
Undertittel
Proceedings of the 103rd Colloquium of the International Astronomical Union, Held in Torun, Poland, August 18–20, 1987
Opplag
Softcover reprint of the original 1st ed. 1988
ISBN
9789401078337
Språk
Engelsk
Vekt
310 gram
Utgivelsesdato
9.11.2011
Forlag
Springer
Antall sider
380