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- W39202206 abstract "A wide-angle search for extended structures (arcs, filaments, cavities etc.) around ca. 400 Galactic planetary nebulae on IRAS SkyView maps revealed several candidates. Some of these dust structures can hardly be explained by chance superpositions of otherwise unrelated objects. They show clear signs of bi- or quadru-polar shape and will, due to their huge dimensions, probably have started to form already in the AGB phase. If so, then the mass-loss in the AGB phase is not spherically symmetric in a number of cases" @default.
- W39202206 created "2016-06-24" @default.
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- W39202206 date "2003-01-01" @default.
- W39202206 modified "2023-09-27" @default.
- W39202206 title "Asymmetric Mass-Loss on the AGB: Examples from IRAS Data" @default.
- W39202206 cites W2055641883 @default.
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- W39202206 doi "https://doi.org/10.1007/978-94-010-0139-7_16" @default.
- W39202206 hasPublicationYear "2003" @default.
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