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Conference Paper: Study of the Galactic Bulge Using New Planetary Nebulae Discovered on the AAO/UKST Hα Survey

TitleStudy of the Galactic Bulge Using New Planetary Nebulae Discovered on the AAO/UKST Hα Survey
Authors
Editors
Editor(s):Sion, EM
KeywordsGalactic Bulge
Planetary Nebulae
Issue Date2005
PublisherSpringer
Citation
White dwarfs: cosmological and galactic probes, 2005, p. 91-93 How to Cite?
AbstractThe AAO/UKST Halpha survey is revealing a substantial new population of Planetary Nebulae (PNe) over the southern Galactic Plane including ~550 in the Bulge. Such objects are excellent tracers for Bulge dynamical studies, are less affected by metallicity bias and have strong emission lines facilitating accurate velocities. We present preliminary results on plans to exploit these significant new Bulge PNe. Until now the relatively small numbers previously known has limited their potential as tracers of galactic structure and as windows to stellar evolution in the critical phase between PNe and White Dwarf (e.g. Zijlstra et al. 1997; Durand et al. 1996, 1998; Beaulieu et al. 1999).
Persistent Identifierhttp://hdl.handle.net/10722/211256
ISBN
Series/Report no.Astrophysics and space science library ; v. 332

 

DC FieldValueLanguage
dc.contributor.authorPeyaud, AEJ-
dc.contributor.authorParker, QA-
dc.contributor.authorAcker, A-
dc.contributor.editorSion, EM-
dc.date.accessioned2015-07-08T03:23:47Z-
dc.date.available2015-07-08T03:23:47Z-
dc.date.issued2005-
dc.identifier.citationWhite dwarfs: cosmological and galactic probes, 2005, p. 91-93-
dc.identifier.isbn9781402036934-
dc.identifier.urihttp://hdl.handle.net/10722/211256-
dc.description.abstractThe AAO/UKST Halpha survey is revealing a substantial new population of Planetary Nebulae (PNe) over the southern Galactic Plane including ~550 in the Bulge. Such objects are excellent tracers for Bulge dynamical studies, are less affected by metallicity bias and have strong emission lines facilitating accurate velocities. We present preliminary results on plans to exploit these significant new Bulge PNe. Until now the relatively small numbers previously known has limited their potential as tracers of galactic structure and as windows to stellar evolution in the critical phase between PNe and White Dwarf (e.g. Zijlstra et al. 1997; Durand et al. 1996, 1998; Beaulieu et al. 1999).-
dc.languageeng-
dc.publisherSpringer-
dc.relation.ispartofWhite dwarfs: cosmological and galactic probes-
dc.relation.ispartofseriesAstrophysics and space science library ; v. 332-
dc.subjectGalactic Bulge-
dc.subjectPlanetary Nebulae-
dc.titleStudy of the Galactic Bulge Using New Planetary Nebulae Discovered on the AAO/UKST Hα Survey-
dc.typeConference_Paper-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.doi10.1007/1-4020-3725-2_11-
dc.identifier.volume332-
dc.identifier.spage91-
dc.identifier.epage93-
dc.publisher.placeDordrecht-

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