The binary central star of the bipolar pre-planetary nebula IRAS 08005−2356 (V510 Pup)
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DOI: 10.1093/mnras/stab2428
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… read more here.
Keywords: pre planetary; v510 pup; iras 08005; 2356 v510 ... See more keywords