Planetary nebulae in the solar neighborhood

David J. Frew; Quentin A. Parker

doi:10.1063/1.2146214

Planetary nebulae in the solar neighborhood

David J. Frew^*, Quentin A. Parker

^*Corresponding author for this work

Faculty of Science and Engineering

Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution › peer-review

5 Citations (Scopus)

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).

Original language	English
Title of host publication	PLANETARY NEBULAE AS ASTRONOMICAL TOOLS: International Conference on Planetary Nebulae as Astronomical Tools
Editors	Ryszard Szczerba, Grazyna Stasinska, Slawomir K. Gorny
Place of Publication	College Park, MD
Publisher	AIP Publishing
Pages	11
Number of pages	1
Volume	804
ISBN (Print)	0735402949, 9780735402942
DOIs	https://doi.org/10.1063/1.2146214
Publication status	Published - 28 Nov 2005
Event	International Conference on Planetary Nebulae as Astronomical Tools - Gdansk, Poland Duration: 28 Jun 2005 → 2 Jul 2005

Other

Other	International Conference on Planetary Nebulae as Astronomical Tools
Country/Territory	Poland
City	Gdansk
Period	28/06/05 → 2/07/05

Keywords

Planetary nebulae: general
Stars: stellar statistics

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10.1063/1.2146214

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@inproceedings{946dba24ce5843538248def737a51bc8,

title = "Planetary nebulae in the solar neighborhood",

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).",

keywords = "Planetary nebulae: general, Stars: stellar statistics",

author = "Frew, {David J.} and Parker, {Quentin A.}",

year = "2005",

month = nov,

day = "28",

doi = "10.1063/1.2146214",

language = "English",

isbn = "0735402949",

volume = "804",

pages = "11",

editor = "Ryszard Szczerba and Grazyna Stasinska and Gorny, {Slawomir K.}",

booktitle = "PLANETARY NEBULAE AS ASTRONOMICAL TOOLS: International Conference on Planetary Nebulae as Astronomical Tools",

publisher = "AIP Publishing",

note = "International Conference on Planetary Nebulae as Astronomical Tools ; Conference date: 28-06-2005 Through 02-07-2005",

}

Frew, DJ & Parker, QA 2005, Planetary nebulae in the solar neighborhood. in R Szczerba, G Stasinska & SK Gorny (eds), PLANETARY NEBULAE AS ASTRONOMICAL TOOLS: International Conference on Planetary Nebulae as Astronomical Tools. vol. 804, AIP Publishing, College Park, MD, pp. 11, International Conference on Planetary Nebulae as Astronomical Tools, Gdansk, Poland, 28/06/05. https://doi.org/10.1063/1.2146214

Planetary nebulae in the solar neighborhood. / Frew, David J.; Parker, Quentin A.
PLANETARY NEBULAE AS ASTRONOMICAL TOOLS: International Conference on Planetary Nebulae as Astronomical Tools. ed. / Ryszard Szczerba; Grazyna Stasinska; Slawomir K. Gorny. Vol. 804 College Park, MD: AIP Publishing, 2005. p. 11.

Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution › peer-review

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AU - Parker, Quentin A.

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N2 - 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).

AB - 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).

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KW - Stars: stellar statistics

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PB - AIP Publishing

CY - College Park, MD

T2 - International Conference on Planetary Nebulae as Astronomical Tools

Y2 - 28 June 2005 through 2 July 2005

ER -

Planetary nebulae in the solar neighborhood

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