Hostname: page-component-76fb5796d-r6qrq Total loading time: 0 Render date: 2024-04-25T08:02:50.511Z Has data issue: false hasContentIssue false

Spectroscopic Variations of the Symbiotic Nova PU VUL

Published online by Cambridge University Press:  12 April 2016

L. Hric
Affiliation:
Astronomical Institute, Slovak Academy of Sciences 059 60 Tatranská Lomnica, Czechoslovakia
D. Chochol
Affiliation:
Astronomical Institute, Slovak Academy of Sciences 059 60 Tatranská Lomnica, Czechoslovakia
B. Kovachev
Affiliation:
Bulgarian Academy of Sciences, National Astronomical Observatory Rozhen, 4700 Smoljan, Bulgaria

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Evidence for formation and subsequent expansion of an A–F supergiant envelope in the very slow symbiotic nova PU Vul caused by quasiperiodic injections of matter from M giant to the A–F supergiant is given.

Type
Session 3. Physics of Individual Objects
Copyright
Copyright © Kluwer 1988

References

Chochol, D., Grygar, J.: 1987, Astrophys. Space Sci. 121, 487.Google Scholar
Kenyon, S.J.: 1986, Astron. J. 21, 563.CrossRefGoogle Scholar
Stellingwerf, R.P.: 1978, Astrophys. J. 224, 953.CrossRefGoogle Scholar