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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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JPL TRS 1992+
JPL TRS 1992+