SHAPING OF NOVA SHELLS - THE CASE OF NOVA V 1974 CYGNI
Expanding shell of Nova V 1974 Cygni consists of two major components: an outer fast - low-mass envelope and an inner slow high-mass envelope. The outer envelope, detected in diffuse enhanced spectra and on radio images, is shaped and accelerated by the fast wind consisting of spherical and polar c...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
Odessa I. I. Mechnykov National University
2017-08-01
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Series: | Odessa Astronomical Publications |
Online Access: | http://oap.onu.edu.ua/article/view/108977 |