File Download

There are no files associated with this item.

  Links for fulltext
     (May Require Subscription)
Supplementary

Article: PHR 1315-6555: a bipolar planetary nebula in the compact Hyades-age open cluster ESO 96-SC04

TitlePHR 1315-6555: a bipolar planetary nebula in the compact Hyades-age open cluster ESO 96-SC04
Authors
Parker, QAFrew, DJMiszalski, BKovacevic, AVFrinchaboy, PMDobbie, PDKöppen, J
Keywordsstars: AGB and post-AGB
white dwarfs
planetary nebulae: individual: PN G305.3-03.1
Issue Date2011
PublisherOxford University press. The Journal's web site is located at http://www.oxfordjournals.org/our_journals/mnras/
Citation
Monthly Notices of the Royal Astronomical Society, 2011, v. 413 n. 3, p. 1835-1844 How to Cite?
DOI: http://dx.doi.org/10.1111/j.1365-2966.2011.18259.x
AbstractWe present a detailed study of a bipolar, possible Type I planetary nebula (PN), PHR 1315-6555 (PN G305.3-03.1), which was discovered as part of the Macquarie/AAO/Strasbourg Halpha planetary nebula project (MASH), and that we considered at the time was an excellent candidate for membership of the distant, compact, intermediate-age open cluster, ESO 96-SC04. The strong evidence for this association is presented here, making this the only known example of a PN physically associated with a Galactic open cluster. Cluster membership is extremely important as it allows for very precise estimates of the fundamental properties of the
Persistent Identifierhttp://hdl.handle.net/10722/211293
ISSN
0035-8711
2023 Impact Factor: 4.7
2023 SCImago Journal Rankings: 1.621
ISI Accession Number ID
WOS:000290487700031

 

DC FieldValueLanguage
dc.contributor.authorParker, QA-
dc.contributor.authorFrew, DJ-
dc.contributor.authorMiszalski, B-
dc.contributor.authorKovacevic, AV-
dc.contributor.authorFrinchaboy, PM-
dc.contributor.authorDobbie, PD-
dc.contributor.authorKöppen, J-
dc.date.accessioned2015-07-08T03:24:16Z-
dc.date.available2015-07-08T03:24:16Z-
dc.date.issued2011-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2011, v. 413 n. 3, p. 1835-1844-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/10722/211293-
dc.description.abstractWe present a detailed study of a bipolar, possible Type I planetary nebula (PN), PHR 1315-6555 (PN G305.3-03.1), which was discovered as part of the Macquarie/AAO/Strasbourg Halpha planetary nebula project (MASH), and that we considered at the time was an excellent candidate for membership of the distant, compact, intermediate-age open cluster, ESO 96-SC04. The strong evidence for this association is presented here, making this the only known example of a PN physically associated with a Galactic open cluster. Cluster membership is extremely important as it allows for very precise estimates of the fundamental properties of the-
dc.languageeng-
dc.publisherOxford University press. 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.subjectstars: AGB and post-AGB-
dc.subjectwhite dwarfs-
dc.subjectplanetary nebulae: individual: PN G305.3-03.1-
dc.titlePHR 1315-6555: a bipolar planetary nebula in the compact Hyades-age open cluster ESO 96-SC04-
dc.typeArticle-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.description.naturelink_to_OA_fulltext-
dc.identifier.doi10.1111/j.1365-2966.2011.18259.x-
dc.identifier.scopuseid_2-s2.0-79955756685-
dc.identifier.volume413-
dc.identifier.issue3-
dc.identifier.spage1835-
dc.identifier.epage1844-
dc.identifier.isiWOS:000290487700031-
dc.identifier.issnl0035-8711-

Export via OAI-PMH Interface in XML Formats

OR

Export to Other Non-XML Formats