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Article: The Hα surface brightness-radius relation: a robust statistical distance indicator for planetary nebulae

TitleThe Hα surface brightness-radius relation: a robust statistical distance indicator for planetary nebulae
Authors
Frew, DJParker, QABojicic, I
KeywordsCircumstellarmatter
H II regions
ISM: bubbles
Planetary nebulae: general
Stars: distances
Techniques: photometric
Issue Date2015
PublisherOxford University press, co-published with Royal Astronomical Society. The Journal's web site is located at http://www.oxfordjournals.org/our_journals/mnras/
Citation
Monthly Notices of the Royal Astronomical Society, 2015, v. 455 n. 2, p. 1459-1488 How to Cite?
DOI: http://dx.doi.org/10.1093/mnras/stv1516
Persistent Identifierhttp://hdl.handle.net/10722/222005
ISSN
0035-8711
2021 Impact Factor: 5.235
2020 SCImago Journal Rankings: 2.058
ISI Accession Number ID
WOS:000368007100026

 

DC FieldValueLanguage
dc.contributor.authorFrew, DJ-
dc.contributor.authorParker, QA-
dc.contributor.authorBojicic, I-
dc.date.accessioned2015-12-21T05:52:04Z-
dc.date.available2015-12-21T05:52:04Z-
dc.date.issued2015-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2015, v. 455 n. 2, p. 1459-1488-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/10722/222005-
dc.languageeng-
dc.publisherOxford University press, co-published with Royal Astronomical Society. The Journal's web site is located at http://www.oxfordjournals.org/our_journals/mnras/-
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society-
dc.rightsThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.-
dc.subjectCircumstellarmatter-
dc.subjectH II regions-
dc.subjectISM: bubbles-
dc.subjectPlanetary nebulae: general-
dc.subjectStars: distances-
dc.subjectTechniques: photometric-
dc.titleThe Hα surface brightness-radius relation: a robust statistical distance indicator for planetary nebulae-
dc.typeArticle-
dc.identifier.emailFrew, DJ: djfrew@hku.hk-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.emailBojicic, I: ibojicic@hku.hk-
dc.identifier.authorityFrew, DJ=rp02013-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.authorityBojicic, I=rp02020-
dc.description.naturepublished_or_final_version-
dc.identifier.doi10.1093/mnras/stv1516-
dc.identifier.scopuseid_2-s2.0-84949603867-
dc.identifier.hkuros256526-
dc.identifier.volume455-
dc.identifier.issue2-
dc.identifier.spage1459-
dc.identifier.epage1488-
dc.identifier.isiWOS:000368007100026-
dc.identifier.issnl0035-8711-

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