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The case of the fastest stellar wind in central stars of planetary nebulae

โœ Scribed by Patrizio Patriarchi; Mario Perinotto


Publisher
Springer Netherlands
Year
1996
Tongue
English
Weight
203 KB
Volume
238
Category
Article
ISSN
0004-640X

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Four minima have been stated and can be interpreted in terms of occulting dust clouds, probably representing dense condensations of the planetary nebula. We derived R = Av1EB-v = 4.0. Photoelektrische UBV-Beobachtungen des Zentralsterns des Planetarischen Nebels NGC 2346, gemessen in 60 Nachten zwis