Do novae have optically thick winds during outburst with large deviations from spherical symmetry?

Context. The evidence for the presence of optically thick winds that are produced by classical novae after optical maximum has been challenged in recent papers. In addition, signs of orbital phase-dependent photometric variations, sometimes seen quite early in the development of nova outbursts, are...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2011-12, Vol.536, p.A97
1. Verfasser:	Friedjung, M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy cataclysmic variables Earth, ocean, space Exact sciences and technology novae outflows stars: individual: V1493 Aql stars: individual: V1500 Cyg stars: winds
Online-Zugang:	Volltext
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