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Conference Paper: The Hα surface brightness - radius plane as a diagnostic tool for photoionized nebulae
| Title | The Hα surface brightness - radius plane as a diagnostic tool for photoionized nebulae |
|---|---|
| Other Titles | The Halpha surface brightness - radius plane as a diagnostic tool for photoionized nebulae |
| Authors | |
| Issue Date | 2016 |
| Publisher | Institute of Physics Publishing. The Journal's web site is located at http://www.iop.org/EJ/journal/conf |
| Citation | The 11th Pacific Rim Conference on Stellar Astrophysics, Hong Kong, 14-17 December 2015. In Journal of Physics: Conference Series, 2016, v. 728, article no. 032015, p. 1-4 How to Cite? |
| Abstract | The Halpha surface brightness - radius (SHalpha-r) relation is a robust distance indicator for planetary nebulae (PNe), further enhanced by different populations of PNe having distinct loci in SHalpha-r space. Other types of photoionized nebulae also plot in quite distinct regions in the SHalpha-r plane, allowing its use as a diagnostic tool. In particular, the nova shells and massive star ejecta (MSE) plot on relatively tight loci illustrating their evolutionary sequences. For the MSE, there is potential to develop a distance indicator for these objects, based on their trend in SHalpha-r space. As high-resolution, narrowband surveys of the nearest galaxies become more commonplace, the SHalpha-r plane is a potentially useful diagnostic tool to help identify the various ionized nebulae in these systems. |
| Description | Conference Theme: Physics and Chemistry of the Late Stages of Stellar Evolution Open Access Article |
| Persistent Identifier | http://hdl.handle.net/10722/232760 |
| ISSN | 2020 SCImago Journal Rankings: 0.210 |
| ISI Accession Number ID |
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Frew, DJ | - |
| dc.contributor.author | Bojicic, I | - |
| dc.contributor.author | Parker, QA | - |
| dc.date.accessioned | 2016-09-20T05:32:07Z | - |
| dc.date.available | 2016-09-20T05:32:07Z | - |
| dc.date.issued | 2016 | - |
| dc.identifier.citation | The 11th Pacific Rim Conference on Stellar Astrophysics, Hong Kong, 14-17 December 2015. In Journal of Physics: Conference Series, 2016, v. 728, article no. 032015, p. 1-4 | - |
| dc.identifier.issn | 1742-6588 | - |
| dc.identifier.uri | http://hdl.handle.net/10722/232760 | - |
| dc.description | Conference Theme: Physics and Chemistry of the Late Stages of Stellar Evolution | - |
| dc.description | Open Access Article | - |
| dc.description.abstract | The Halpha surface brightness - radius (SHalpha-r) relation is a robust distance indicator for planetary nebulae (PNe), further enhanced by different populations of PNe having distinct loci in SHalpha-r space. Other types of photoionized nebulae also plot in quite distinct regions in the SHalpha-r plane, allowing its use as a diagnostic tool. In particular, the nova shells and massive star ejecta (MSE) plot on relatively tight loci illustrating their evolutionary sequences. For the MSE, there is potential to develop a distance indicator for these objects, based on their trend in SHalpha-r space. As high-resolution, narrowband surveys of the nearest galaxies become more commonplace, the SHalpha-r plane is a potentially useful diagnostic tool to help identify the various ionized nebulae in these systems. | - |
| dc.language | eng | - |
| dc.publisher | Institute of Physics Publishing. The Journal's web site is located at http://www.iop.org/EJ/journal/conf | - |
| dc.relation.ispartof | Journal of Physics: Conference Series | - |
| dc.rights | Journal of Physics: Conference Series. Copyright © Institute of Physics Publishing. | - |
| dc.rights | This is an author-created, un-copyedited version of an article published in [insert name of journal]. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at http://dx.doi.org/[insert DOI]. | - |
| dc.title | The Hα surface brightness - radius plane as a diagnostic tool for photoionized nebulae | - |
| dc.title.alternative | The Halpha surface brightness - radius plane as a diagnostic tool for photoionized nebulae | - |
| dc.type | Conference_Paper | - |
| dc.identifier.email | Frew, DJ: djfrew@hku.hk | - |
| dc.identifier.email | Bojicic, I: ibojicic@hku.hk | - |
| dc.identifier.email | Parker, QA: physhead@hku.hk | - |
| dc.identifier.authority | Frew, DJ=rp02013 | - |
| dc.identifier.authority | Bojicic, I=rp02020 | - |
| dc.identifier.authority | Parker, QA=rp02017 | - |
| dc.description.nature | link_to_OA_fulltext | - |
| dc.identifier.doi | 10.1088/1742-6596/728/3/032015 | - |
| dc.identifier.scopus | eid_2-s2.0-84989316499 | - |
| dc.identifier.hkuros | 266100 | - |
| dc.identifier.volume | 728, article no. 032015 | - |
| dc.identifier.spage | 1 | - |
| dc.identifier.epage | 4 | - |
| dc.identifier.isi | WOS:000397958000024 | - |
| dc.publisher.place | United Kingdom | - |
| dc.identifier.issnl | 1742-6588 | - |