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- W4300544797 abstract "The question of what physical mechanisms shape planetary nebulae into their observed morphologies remains open. However, intensified efforts since the last meeting in this series, Asymmetrical Planetary Nebulae IV, in July 2007 have yielded some excellent results. In this review we concentrate on those developments that have taken place in the last three years, with emphasis on results obtained since the review by De Marco (2009)." @default.
- W4300544797 created "2022-10-03" @default.
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- W4300544797 date "2010-10-19" @default.
- W4300544797 modified "2023-09-27" @default.
- W4300544797 title "New results on planetary nebula shaping and stellar binarity" @default.
- W4300544797 doi "https://doi.org/10.48550/arxiv.1010.3802" @default.
- W4300544797 hasPublicationYear "2010" @default.
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