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Article: Discovery of new low-excitation planetary nebulae

TitleDiscovery of new low-excitation planetary nebulae
Authors
KeywordsPlanetary nebulae: general
Stars: AGB and post-AGB
Surveys
Issue Date2014
PublisherEDP Sciences. The Journal's web site is located at http://www.aanda.org
Citation
Astronomy & Astrophysics, 2014, v. 563, article no. A63 How to Cite?
AbstractWe report a multi-wavelength study of four new planetary nebula (PN) candidates selected from the INT/WFC Photometric Hα Survey of the Northern Galactic Plane (IPHAS) and Deep Sky Hunter (DSH) catalogues. We present mid-resolution optical spectra of these PNs. The PN status of our sample was confirmed by optical narrow-band images and mid-resolution spectra. Based on the locations of these objects in the log(Hα/[N II]) versus log(Hα/[S II]) diagnostic diagram, we conclude that these sources are evolved low-excitation PNs. The optical and infrared appearances of these newly discovered PNs are discussed. Three of the new nebulae studied here are detected in infrared and have low infrared-to-radio flux ratios, probably suggesting that they are evolved. Furthermore, we derive the dynamical ages and distances of these nebulae and study the spectral energy distribution for one of them with extensive infrared archival data.
Persistent Identifierhttp://hdl.handle.net/10722/198064
ISSN
2023 Impact Factor: 5.4
2023 SCImago Journal Rankings: 1.896
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorHsia, Cen_US
dc.contributor.authorZhang, Yen_US
dc.date.accessioned2014-06-25T02:44:07Z-
dc.date.available2014-06-25T02:44:07Z-
dc.date.issued2014en_US
dc.identifier.citationAstronomy & Astrophysics, 2014, v. 563, article no. A63en_US
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/10722/198064-
dc.description.abstractWe report a multi-wavelength study of four new planetary nebula (PN) candidates selected from the INT/WFC Photometric Hα Survey of the Northern Galactic Plane (IPHAS) and Deep Sky Hunter (DSH) catalogues. We present mid-resolution optical spectra of these PNs. The PN status of our sample was confirmed by optical narrow-band images and mid-resolution spectra. Based on the locations of these objects in the log(Hα/[N II]) versus log(Hα/[S II]) diagnostic diagram, we conclude that these sources are evolved low-excitation PNs. The optical and infrared appearances of these newly discovered PNs are discussed. Three of the new nebulae studied here are detected in infrared and have low infrared-to-radio flux ratios, probably suggesting that they are evolved. Furthermore, we derive the dynamical ages and distances of these nebulae and study the spectral energy distribution for one of them with extensive infrared archival data.-
dc.languageengen_US
dc.publisherEDP Sciences. The Journal's web site is located at http://www.aanda.org-
dc.relation.ispartofAstronomy & Astrophysicsen_US
dc.rights© ESO 2014. The original publication is available at https://doi.org/10.1051/0004-6361/201322500-
dc.subjectPlanetary nebulae: general-
dc.subjectStars: AGB and post-AGB-
dc.subjectSurveys-
dc.titleDiscovery of new low-excitation planetary nebulaeen_US
dc.typeArticleen_US
dc.identifier.emailHsia, C: xiazh@hku.hken_US
dc.identifier.emailZhang, Y: zhangy96@hku.hken_US
dc.identifier.authorityHsia, C=rp00706en_US
dc.identifier.authorityZhang, Y=rp00841en_US
dc.description.naturepublished_or_final_version-
dc.identifier.doi10.1051/0004-6361/201322500-
dc.identifier.scopuseid_2-s2.0-84896761032-
dc.identifier.hkuros229127en_US
dc.identifier.volume563en_US
dc.identifier.spagearticle no. A63-
dc.identifier.epagearticle no. A63-
dc.identifier.isiWOS:000333798000063-
dc.publisher.placeFrance-
dc.identifier.issnl0004-6361-

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