File Download

There are no files associated with this item.

  Links for fulltext
     (May Require Subscription)
Supplementary

Article: 400 new planetary nebulae in the galactic bulge

Title400 new planetary nebulae in the galactic bulge
Authors
Acker, AgnèsPeyaud, Alan E JParker, Quentin A.
KeywordsPlanetary nebulae
Galactic bulge
Issue Date2006
Citation
Proceedings of the International Astronomical Union, 2006, v. 2, n. 234, p. 355-356 How to Cite?
DOI: http://dx.doi.org/10.1017/S1743921306003218
AbstractAbout 500 MASH(Macquarie/AAO/Strasbourg Hα planetary nebula, project) PNe were discovered towards the galactic bulge (Parker et al. 2006). For 405 MASH PNe with a diameter < 35 arcsec, we obtain surface brightness, diameter and dynamical age of the nebulae. From line intensity ratios of 133 GBPN observed with the 6dF device, we obtain their density and ionized mass, and their central star temperatures. We discover 15 bipolar and/or nitrogen-rich GBPNe having probably massive stellar progenitors (Peyaud, 2005). © 2006 International Astronomical Union.
Persistent Identifierhttp://hdl.handle.net/10722/208868
ISSN
1743-9213
2020 SCImago Journal Rankings: 0.124

 

DC FieldValueLanguage
dc.contributor.authorAcker, Agnès-
dc.contributor.authorPeyaud, Alan E J-
dc.contributor.authorParker, Quentin A.-
dc.date.accessioned2015-03-23T02:02:00Z-
dc.date.available2015-03-23T02:02:00Z-
dc.date.issued2006-
dc.identifier.citationProceedings of the International Astronomical Union, 2006, v. 2, n. 234, p. 355-356-
dc.identifier.issn1743-9213-
dc.identifier.urihttp://hdl.handle.net/10722/208868-
dc.description.abstractAbout 500 MASH(Macquarie/AAO/Strasbourg Hα planetary nebula, project) PNe were discovered towards the galactic bulge (Parker et al. 2006). For 405 MASH PNe with a diameter < 35 arcsec, we obtain surface brightness, diameter and dynamical age of the nebulae. From line intensity ratios of 133 GBPN observed with the 6dF device, we obtain their density and ionized mass, and their central star temperatures. We discover 15 bipolar and/or nitrogen-rich GBPNe having probably massive stellar progenitors (Peyaud, 2005). © 2006 International Astronomical Union.-
dc.languageeng-
dc.relation.ispartofProceedings of the International Astronomical Union-
dc.subjectPlanetary nebulae-
dc.subjectGalactic bulge-
dc.title400 new planetary nebulae in the galactic bulge-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1017/S1743921306003218-
dc.identifier.scopuseid_2-s2.0-33845526976-
dc.identifier.volume2-
dc.identifier.issue234-
dc.identifier.spage355-
dc.identifier.epage356-
dc.identifier.eissn1743-9221-
dc.identifier.issnl1743-9213-

Export via OAI-PMH Interface in XML Formats

OR

Export to Other Non-XML Formats