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Discovery of a Remarkable Point-Symmetric Protoplanetary Nebula: HST Imaging of IRAS04296+3429

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dc.contributor.author Sahai, R. en_US
dc.date.accessioned 2004-09-24T17:07:06Z
dc.date.available 2004-09-24T17:07:06Z
dc.date.issued 1999-09 en_US
dc.identifier.citation Astrophysical Journal en_US
dc.identifier.citation USA en_US
dc.identifier.clearanceno 99-1676 en_US
dc.identifier.uri http://hdl.handle.net/2014/18209
dc.description.abstract Most planetary nebulae (PN) show significant departures from sperical symmetry, whereas the circumstellar envelopes (CSEs) of their progenitor AGB stars appear spherically symmetric. en_US
dc.format.extent 602503 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other planetary nebulae stars AGB post AGB mass-loss circumstellar matter en_US
dc.title Discovery of a Remarkable Point-Symmetric Protoplanetary Nebula: HST Imaging of IRAS04296+3429 en_US


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