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Conference Paper: Planetary nebulae in the solar neighborhood

TitlePlanetary nebulae in the solar neighborhood
Authors
Frew, David J.Parker, Quentin A.
KeywordsPlanetary nebulae: general
Stars: stellar statistics
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. 11 How to Cite?
DOI: http://dx.doi.org/10.1063/1.2146214
AbstractThe AAO/UKST Hα Survey has been used to discover a number of new, large, nearby planetary nebulae (PNe) These discoveries, combined with a critical re-analysis of all previously known large PNe, have allowed the compilation of a relatively complete census of PNe in the solar neighbourhood within 1.0 kpc. Distances are based in part on a new Hα surface brightness - radius relation. The census is relatively bias-free, and will provide more accurate estimates of the PN formation rate, average PN lifetime, and the total number of PNe in the Galaxy, as well as a first look at the faint end of the PN luminosity function (PNLF). © 2005 American Institute of Physics.
Persistent Identifierhttp://hdl.handle.net/10722/208865
ISSN
0094-243X
2020 SCImago Journal Rankings: 0.177

 

DC FieldValueLanguage
dc.contributor.authorFrew, David J.-
dc.contributor.authorParker, Quentin A.-
dc.date.accessioned2015-03-23T02:01:59Z-
dc.date.available2015-03-23T02:01:59Z-
dc.date.issued2005-
dc.identifier.citationAIP Conference Proceedings, 2005, v. 804 n. 1, p. 11-
dc.identifier.issn0094-243X-
dc.identifier.urihttp://hdl.handle.net/10722/208865-
dc.description.abstractThe AAO/UKST Hα Survey has been used to discover a number of new, large, nearby planetary nebulae (PNe) These discoveries, combined with a critical re-analysis of all previously known large PNe, have allowed the compilation of a relatively complete census of PNe in the solar neighbourhood within 1.0 kpc. Distances are based in part on a new Hα surface brightness - radius relation. The census is relatively bias-free, and will provide more accurate estimates of the PN formation rate, average PN lifetime, and the total number of PNe in the Galaxy, as well as a first look at the faint end of the PN luminosity function (PNLF). © 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.subjectPlanetary nebulae: general-
dc.subjectStars: stellar statistics-
dc.titlePlanetary nebulae in the solar neighborhood-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1063/1.2146214-
dc.identifier.scopuseid_2-s2.0-33751219559-
dc.identifier.volume804-
dc.identifier.issue1-
dc.identifier.spage11-
dc.identifier.epage11-
dc.identifier.eissn1551-7616-
dc.identifier.issnl0094-243X-

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