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Conference Paper: A new population of planetary nebulae discovered in the large magellanic cloud

TitleA new population of planetary nebulae discovered in the large magellanic cloud
Authors
Reid, Warren A.Parker, Quentin A.
KeywordsLarge magellanic cloud
Hα survey
Planetary nebula
Issue Date2005
PublisherAmerican Institute of Physics. The Journal's web site is located at http://proceedings.aip.org/
Citation
AIP Conference Proceedings, 2005, v. 804 n. 1, p. 12 How to Cite?
DOI: http://dx.doi.org/10.1063/1.2146215
AbstractWe report discovery of ∼600 planetary nebulae (PNe) in the central 25 sq. degree region of the Large Magellanic Cloud (LMC). Candidates were found on a multi-exposure Hα and short red (SR) combined UK Schmidt Telescope (UKST) map. Confirmatory 2dF fibre spectroscopy on the Anglo-Australian Telescope (AAT) has almost tripled the number of PNe in the LMC central bar region. This new population will have important implications for the PN luminosity function and will provide improved kinematics, refined abundance gradients and a better picture of chemical evolution. © 2005 American Institute of Physics.
Persistent Identifierhttp://hdl.handle.net/10722/208867
ISSN
0094-243X
2020 SCImago Journal Rankings: 0.177

 

DC FieldValueLanguage
dc.contributor.authorReid, Warren A.-
dc.contributor.authorParker, Quentin A.-
dc.date.accessioned2015-03-23T02:02:00Z-
dc.date.available2015-03-23T02:02:00Z-
dc.date.issued2005-
dc.identifier.citationAIP Conference Proceedings, 2005, v. 804 n. 1, p. 12-
dc.identifier.issn0094-243X-
dc.identifier.urihttp://hdl.handle.net/10722/208867-
dc.description.abstractWe report discovery of ∼600 planetary nebulae (PNe) in the central 25 sq. degree region of the Large Magellanic Cloud (LMC). Candidates were found on a multi-exposure Hα and short red (SR) combined UK Schmidt Telescope (UKST) map. Confirmatory 2dF fibre spectroscopy on the Anglo-Australian Telescope (AAT) has almost tripled the number of PNe in the LMC central bar region. This new population will have important implications for the PN luminosity function and will provide improved kinematics, refined abundance gradients and a better picture of chemical evolution. © 2005 American Institute of Physics.-
dc.languageeng-
dc.publisherAmerican Institute of Physics. The Journal's web site is located at http://proceedings.aip.org/-
dc.relation.ispartofAIP Conference Proceedings-
dc.subjectLarge magellanic cloud-
dc.subjectHα survey-
dc.subjectPlanetary nebula-
dc.titleA new population of planetary nebulae discovered in the large magellanic cloud-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1063/1.2146215-
dc.identifier.scopuseid_2-s2.0-33751233541-
dc.identifier.volume804-
dc.identifier.issue1-
dc.identifier.spage12-
dc.identifier.epage12-
dc.identifier.eissn1551-7616-
dc.identifier.issnl0094-243X-

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