An Emission Line Analysis of MASH Galactic PNe

Details An Emission Line Analysis of MASH Galactic PNe An Emission Line Analysis of MASH Galactic PNe

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..404..337k&link_type=abstract

The Eighth Pacific Rim Conference on Stellar Astrophysics: A Tribute to Kam-Ching Leung ASP Conference Series, Vol. 404, proceed

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We present preliminary spectrophotometric results for Galactic Planetary Nebulae (PNe) in the Macquarie/AAO/Strasbourg H-alpha Planetary Nebulae Catalogue (MASH) \citep{P}. MASH PNe generally represent the more evolved end of the luminosity function than previous catalogues due to the inherent depth and resolution of the data. Excitation classes are derived for the sample from the new available spectroscopy and confirm trends established by \citet{RP}. The excitation classes are compared to other observed PNe properties such as morphology, electron density and Galactic location.

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