Very Young Proto-Planetary Nebulae: An Optical Imaging and Spectroscopic Survey

Details Very Young Proto-Planetary Nebulae: An Optical Imaging and Spectroscopic Survey Very Young Proto-Planetary Nebulae: An Optical Imaging and Spectroscopic Survey

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..313...32s&link_type=abstract

Asymmetrical Planetary Nebulae III: Winds, Structure and the Thunderbird, Proceedings of the conference held 28 July - 1 August

Astronomy and Astrophysics

Astronomy

9

Scientific paper

Proto-Planetary nebulae (pPNe) -- objects in transition between the AGB and planetary nebula (PN) evolutionary phases -- hold the key to our understanding of the dramatic transformations in morphology and kinematics of mass-ejecta during the very late stages of stellar evolution for ˜1-8ms stars. We summarise here the first results from the optical part of our multiwavelength survey of pPNe candidates, which include the discovery of many bipolar/ multipolar nebulae and very fast, most likely collimated, post-AGB outflows.

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