Inspecting infrared properties of proto- and young planetary nebulae

Details Inspecting infrared properties of proto- and young planetary nebulae Inspecting infrared properties of proto- and young planetary nebulae

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sptz.prop30036f&link_type=abstract

Spitzer Proposal ID #30036

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Scientific paper

We propose IRAC and IRS observations of a sample of proto- and young Planetary Nebulae to study stellar ejecta properties. In particular, our previous radio observations give us the possibility to compare ionized (radio detected) and non-ionized (non radio detected) envelopes in a sample of transition objects. Such a study will allow us, among other things, to investigate the effect of ionization on nebular envelopes, in relation to their chemical content and shapes.

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