File Download
There are no files associated with this item.
Links for fulltext
(May Require Subscription)
- Publisher Website: 10.1063/1.2146214
- Scopus: eid_2-s2.0-33751219559
- Find via
Supplementary
-
Citations:
- Scopus: 0
- Appears in Collections:
Conference Paper: Planetary nebulae in the solar neighborhood
Title | Planetary nebulae in the solar neighborhood |
---|---|
Authors | |
Keywords | Planetary nebulae: general Stars: stellar statistics |
Issue Date | 2005 |
Publisher | American Institute of Physics. The Journal's web site is located at http://proceedings.aip.org/ |
Citation | AIP Conference Proceedings, 2005, v. 804 n. 1, p. 11 How to Cite? |
Abstract | The AAO/UKST Hα Survey has been used to discover a number of new, large, nearby planetary nebulae (PNe) These discoveries, combined with a critical re-analysis of all previously known large PNe, have allowed the compilation of a relatively complete census of PNe in the solar neighbourhood within 1.0 kpc. Distances are based in part on a new Hα surface brightness - radius relation. The census is relatively bias-free, and will provide more accurate estimates of the PN formation rate, average PN lifetime, and the total number of PNe in the Galaxy, as well as a first look at the faint end of the PN luminosity function (PNLF). © 2005 American Institute of Physics. |
Persistent Identifier | http://hdl.handle.net/10722/208865 |
ISSN | 2023 SCImago Journal Rankings: 0.152 |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Frew, David J. | - |
dc.contributor.author | Parker, Quentin A. | - |
dc.date.accessioned | 2015-03-23T02:01:59Z | - |
dc.date.available | 2015-03-23T02:01:59Z | - |
dc.date.issued | 2005 | - |
dc.identifier.citation | AIP Conference Proceedings, 2005, v. 804 n. 1, p. 11 | - |
dc.identifier.issn | 0094-243X | - |
dc.identifier.uri | http://hdl.handle.net/10722/208865 | - |
dc.description.abstract | The AAO/UKST Hα Survey has been used to discover a number of new, large, nearby planetary nebulae (PNe) These discoveries, combined with a critical re-analysis of all previously known large PNe, have allowed the compilation of a relatively complete census of PNe in the solar neighbourhood within 1.0 kpc. Distances are based in part on a new Hα surface brightness - radius relation. The census is relatively bias-free, and will provide more accurate estimates of the PN formation rate, average PN lifetime, and the total number of PNe in the Galaxy, as well as a first look at the faint end of the PN luminosity function (PNLF). © 2005 American Institute of Physics. | - |
dc.language | eng | - |
dc.publisher | American Institute of Physics. The Journal's web site is located at http://proceedings.aip.org/ | - |
dc.relation.ispartof | AIP Conference Proceedings | - |
dc.subject | Planetary nebulae: general | - |
dc.subject | Stars: stellar statistics | - |
dc.title | Planetary nebulae in the solar neighborhood | - |
dc.type | Conference_Paper | - |
dc.description.nature | link_to_subscribed_fulltext | - |
dc.identifier.doi | 10.1063/1.2146214 | - |
dc.identifier.scopus | eid_2-s2.0-33751219559 | - |
dc.identifier.volume | 804 | - |
dc.identifier.issue | 1 | - |
dc.identifier.spage | 11 | - |
dc.identifier.epage | 11 | - |
dc.identifier.eissn | 1551-7616 | - |
dc.identifier.issnl | 0094-243X | - |