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Conference Paper: An Emission Line Analysis of MASH Galactic PNe
| Title | An Emission Line Analysis of MASH Galactic PNe |
|---|---|
| Authors | |
| Editors | Editor(s):Soonthornthum, B |
| Issue Date | 2008 |
| Citation | The 8th Pacific Rim Conference on Stellar Astrophysics: A Tribute to Kam-Ching Leung ASP Conference Series, Vol. 404, Phuket, Thailand, 5-9 May 2008, p. 337-337 How to Cite? |
| Abstract | We present preliminary spectrophotometric results for Galactic Planetary Nebulae (PNe) in the Macquarie/AAO/Strasbourg H-alpha Planetary Nebulae Catalogue (MASH) \citep{P}. MASH PNe generally represent the more evolved end of the luminosity function than previous catalogues due to the inherent depth and resolution of the data. Excitation classes are derived for the sample from the new available spectroscopy and confirm trends established by \citet{RP}. The excitation classes are compared to other observed PNe properties such as morphology, electron density and Galactic location. |
| Persistent Identifier | http://hdl.handle.net/10722/211249 |
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Kovacevic, A | - |
| dc.contributor.author | Parker, QA | - |
| dc.contributor.author | Komonjinda, S | - |
| dc.contributor.author | Cheng, KS | - |
| dc.contributor.author | Leung, KC | - |
| dc.contributor.editor | Soonthornthum, B | - |
| dc.date.accessioned | 2015-07-08T03:23:41Z | - |
| dc.date.available | 2015-07-08T03:23:41Z | - |
| dc.date.issued | 2008 | - |
| dc.identifier.citation | The 8th Pacific Rim Conference on Stellar Astrophysics: A Tribute to Kam-Ching Leung ASP Conference Series, Vol. 404, Phuket, Thailand, 5-9 May 2008, p. 337-337 | - |
| dc.identifier.uri | http://hdl.handle.net/10722/211249 | - |
| dc.description.abstract | We present preliminary spectrophotometric results for Galactic Planetary Nebulae (PNe) in the Macquarie/AAO/Strasbourg H-alpha Planetary Nebulae Catalogue (MASH) \citep{P}. MASH PNe generally represent the more evolved end of the luminosity function than previous catalogues due to the inherent depth and resolution of the data. Excitation classes are derived for the sample from the new available spectroscopy and confirm trends established by \citet{RP}. The excitation classes are compared to other observed PNe properties such as morphology, electron density and Galactic location. | - |
| dc.language | eng | - |
| dc.relation.ispartof | The 8th Pacific Rim Conference on Stellar Astrophysics: A Tribute to Kam-Ching Leung ASP Conference Series | - |
| dc.title | An Emission Line Analysis of MASH Galactic PNe | - |
| dc.type | Conference_Paper | - |
| dc.identifier.email | Parker, QA: quentinp@hku.hk | - |
| dc.identifier.authority | Parker, QA=rp02017 | - |
| dc.identifier.volume | 404 | - |
| dc.identifier.spage | 337 | - |
| dc.identifier.epage | 337 | - |