The binary central star of the bipolar pre-planetary nebula IRAS 08005−2356 (V510 Pup)

ABSTRACT Current models predict that binary interactions are a major ingredient in the formation of bipolar planetary nebulae (PNe) and pre-planetary nebulae (PPNe). Despite years of radial velocity (RV) monitoring, the paucity of known binaries amongst the latter systems means data are insufficient...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2021-12, Vol.508 (2), p.2226-2235
Hauptverfasser: Manick, Rajeev, Miszalski, Brent, Kamath, Devika, Whitelock, Patricia A, Van Winckel, Hans, Hrivnak, Bruce J, Barlow, Brad N, Mohamed, Shazrene
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Sprache:eng
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