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Conference Paper: Deep study of the Galactic Bulge using new Planetary Nebulae discovered on the AAO/UKST Halpha survey

TitleDeep study of the Galactic Bulge using new Planetary Nebulae discovered on the AAO/UKST Halpha survey
Authors
Editors
Editor(s):Combes, F
Issue Date2003
Citation
SF2A-2003: Semaine de l'Astrophysique Francaise, Bordeaux, France, 16-20 June 2003, p. 311-311 How to Cite?
AbstractThe exploitation of data from the Halpha southern survey and from the spectroscopic survey of newly discovered planetary nebulae (PN) is focussed on the 1500 PN of the galactic bulge, with the following objectives: -- history of expansion linked to the evolutive models as a function of progenitor mass; -- spatial distribution and kinematics to constrain the dynamics.
Persistent Identifierhttp://hdl.handle.net/10722/211263

 

DC FieldValueLanguage
dc.contributor.authorPeyaud, AEJ-
dc.contributor.authorParker, QA-
dc.contributor.authorAcker, A-
dc.contributor.authorBarret, D-
dc.contributor.authorContini, T-
dc.contributor.authorPagani, L-
dc.contributor.editorCombes, F-
dc.date.accessioned2015-07-08T03:23:53Z-
dc.date.available2015-07-08T03:23:53Z-
dc.date.issued2003-
dc.identifier.citationSF2A-2003: Semaine de l'Astrophysique Francaise, Bordeaux, France, 16-20 June 2003, p. 311-311-
dc.identifier.urihttp://hdl.handle.net/10722/211263-
dc.description.abstractThe exploitation of data from the Halpha southern survey and from the spectroscopic survey of newly discovered planetary nebulae (PN) is focussed on the 1500 PN of the galactic bulge, with the following objectives: -- history of expansion linked to the evolutive models as a function of progenitor mass; -- spatial distribution and kinematics to constrain the dynamics.-
dc.languageeng-
dc.relation.ispartofSF2A-2003: Semaine de l'Astrophysique Francaise-
dc.titleDeep study of the Galactic Bulge using new Planetary Nebulae discovered on the AAO/UKST Halpha survey-
dc.typeConference_Paper-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.spage311-
dc.identifier.epage311-

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