File Download

There are no files associated with this item.

Supplementary

Conference Paper: Central Stars of MASH Planetary Nebulae

TitleCentral Stars of MASH Planetary Nebulae
Authors
Miszalski, BAcker, AParker, QA
Editors
Editor(s):Werner, A
Issue Date2008
PublisherAstronomical Society of the Pacific
Citation
Hydrogen-Deficient Stars, ASP Conference Series, Vol. 391, Tübingen, Germany, 17-21 September, 2007, p. 181-182 How to Cite?
AbstractThe AAO/UKST Halpha survey of the Southern Galactic Plane has produced large numbers of new planetary nebulae (PN). These are contained in the Macquarie/AAO/Strasbourg Halpha catalogue (MASH) and a supplementary catalogue called MASH-II. The large combined sample of ˜1200 PN offers many new central stars (CSPN) for study. We outline a small portion of these CSPN that have been observed spectroscopically with particular focus on Wolf-Rayet CSPN, of which we find and classify around 30 new objects.
Persistent Identifierhttp://hdl.handle.net/10722/211251
ISBN
9781583816523
Series/Report no.Astronomical Society of the Pacific conference series ; v. 391

 

DC FieldValueLanguage
dc.contributor.authorMiszalski, B-
dc.contributor.authorAcker, A-
dc.contributor.authorParker, QA-
dc.contributor.editorWerner, A-
dc.date.accessioned2015-07-08T03:23:43Z-
dc.date.available2015-07-08T03:23:43Z-
dc.date.issued2008-
dc.identifier.citationHydrogen-Deficient Stars, ASP Conference Series, Vol. 391, Tübingen, Germany, 17-21 September, 2007, p. 181-182-
dc.identifier.isbn9781583816523-
dc.identifier.urihttp://hdl.handle.net/10722/211251-
dc.description.abstractThe AAO/UKST Halpha survey of the Southern Galactic Plane has produced large numbers of new planetary nebulae (PN). These are contained in the Macquarie/AAO/Strasbourg Halpha catalogue (MASH) and a supplementary catalogue called MASH-II. The large combined sample of ˜1200 PN offers many new central stars (CSPN) for study. We outline a small portion of these CSPN that have been observed spectroscopically with particular focus on Wolf-Rayet CSPN, of which we find and classify around 30 new objects.-
dc.languageeng-
dc.publisherAstronomical Society of the Pacific-
dc.relation.ispartofHydrogen-Deficient Stars, ASP Conference Series-
dc.relation.ispartofseriesAstronomical Society of the Pacific conference series ; v. 391-
dc.titleCentral Stars of MASH Planetary Nebulae-
dc.typeConference_Paper-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.spage181-
dc.identifier.epage182-
dc.publisher.placeSan Francisco-

Export via OAI-PMH Interface in XML Formats

OR

Export to Other Non-XML Formats