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Conference Paper: An Emission Line Analysis of MASH Galactic PNe

TitleAn Emission Line Analysis of MASH Galactic PNe
Authors
Kovacevic, AParker, Q
Issue Date1-Jan-2009
PublisherASTRONOMICAL SOC PACIFIC
AbstractWe present preliminary spectrophotometric results for Galactic Planetary Nebulae (PNe) in the Macquarie/AAO/Strasbourg H-alpha Planetary Nebulae Catalogue (MASH) (Parker et al. 2006). 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 Reid & Parker (2006). The excitation classes are compared to other observed PNe properties such as morphology, electron density and Galactic location.
Persistent Identifierhttp://hdl.handle.net/10722/342813
ISBN
978-1-58381-685-1
ISI Accession Number ID
WOS:000271628900066

 

DC FieldValueLanguage
dc.contributor.authorKovacevic, A-
dc.contributor.authorParker, Q-
dc.date.accessioned2024-05-02T03:06:03Z-
dc.date.available2024-05-02T03:06:03Z-
dc.date.issued2009-01-01-
dc.identifier.isbn978-1-58381-685-1-
dc.identifier.urihttp://hdl.handle.net/10722/342813-
dc.description.abstractWe present preliminary spectrophotometric results for Galactic Planetary Nebulae (PNe) in the Macquarie/AAO/Strasbourg H-alpha Planetary Nebulae Catalogue (MASH) (Parker et al. 2006). 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 Reid & Parker (2006). The excitation classes are compared to other observed PNe properties such as morphology, electron density and Galactic location.-
dc.languageeng-
dc.publisherASTRONOMICAL SOC PACIFIC-
dc.relation.ispartof8th Pacific Rim Conference on Stellar Astrophysics (05/05/2008, Phuket)-
dc.titleAn Emission Line Analysis of MASH Galactic PNe-
dc.typeConference_Paper-
dc.identifier.volume404-
dc.identifier.spage337-
dc.identifier.epage339-
dc.identifier.isiWOS:000271628900066-
dc.publisher.placeSAN FRANCISCO-

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