File Download

There are no files associated with this item.

  Links for fulltext
     (May Require Subscription)
Supplementary

Conference Paper: Newly discovered halos and outer features around southern planetary nebulae

TitleNewly discovered halos and outer features around southern planetary nebulae
Authors
Keywordsstars: evolution
Planetary nebulae: general
stars: AGB and post-AGB
ISM: general
Issue Date2011
Citation
Proceedings of the International Astronomical Union, 2011, v. 7, n. S283, p. 362-363 How to Cite?
AbstractWe have used the SuperCOSMOS Hα Survey to look for faint outer structures such as halos, ansae and jets around known planetary nebulae across 4000 square degrees of the southern Milky Way. Our search will contribute to a more accurate census of these features in the Galactic PN population. Candidate common-envelope PNe have also been identified on the basis of their microstructures. We also intend to determine more reliable distances for these PNe, which should allow a much better statistical basis for the post-AGB total mass budget. Our survey offers fresh scope to address this important issue. © 2012 International Astronomical Union.
Persistent Identifierhttp://hdl.handle.net/10722/208956
ISSN
2015 SCImago Journal Rankings: 0.105

 

DC FieldValueLanguage
dc.contributor.authorFrew, David J.-
dc.contributor.authorBojičić, Ivan S.-
dc.contributor.authorParker, Quentin A.-
dc.date.accessioned2015-03-23T02:02:21Z-
dc.date.available2015-03-23T02:02:21Z-
dc.date.issued2011-
dc.identifier.citationProceedings of the International Astronomical Union, 2011, v. 7, n. S283, p. 362-363-
dc.identifier.issn1743-9213-
dc.identifier.urihttp://hdl.handle.net/10722/208956-
dc.description.abstractWe have used the SuperCOSMOS Hα Survey to look for faint outer structures such as halos, ansae and jets around known planetary nebulae across 4000 square degrees of the southern Milky Way. Our search will contribute to a more accurate census of these features in the Galactic PN population. Candidate common-envelope PNe have also been identified on the basis of their microstructures. We also intend to determine more reliable distances for these PNe, which should allow a much better statistical basis for the post-AGB total mass budget. Our survey offers fresh scope to address this important issue. © 2012 International Astronomical Union.-
dc.languageeng-
dc.relation.ispartofProceedings of the International Astronomical Union-
dc.subjectstars: evolution-
dc.subjectPlanetary nebulae: general-
dc.subjectstars: AGB and post-AGB-
dc.subjectISM: general-
dc.titleNewly discovered halos and outer features around southern planetary nebulae-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1017/S174392131201143X-
dc.identifier.scopuseid_2-s2.0-84865796467-
dc.identifier.volume7-
dc.identifier.issueS283-
dc.identifier.spage362-
dc.identifier.epage363-
dc.identifier.eissn1743-9221-

Export via OAI-PMH Interface in XML Formats


OR


Export to Other Non-XML Formats