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Conference Paper: HASH: the Hong Kong/AAO/Strasbourg Hα planetary nebula database

TitleHASH: the Hong Kong/AAO/Strasbourg Hα planetary nebula database
Authors
Issue Date2016
PublisherInstitute of Physics Publishing. The Journal's web site is located at http://www.iop.org/EJ/journal/conf
Citation
11th Pacific Rim Conference on Stellar Astrophysics: Physics and Chemistry of the Late Stages of Stellar Evolution, Hong Kong, PR China, 14–17 December 2015. In Journal of Physics: Conference Series, 2016, v. 728, article no. 032008 How to Cite?
AbstractBy incorporating our major recent discoveries with re-measured and verified contents of existing catalogues we provide, for the first time, an accessible, reliable, on-line SQL database for essential, up-to date information for all known Galactic planetary nebulae (PNe). We have attempted to: i) reliably remove PN mimics/false ID's that have biased previous studies and ii) provide accurate positions, sizes, morphologies, multi-wavelength imagery and spectroscopy. We also provide a link to CDS/Vizier for the archival history of each object and other valuable links to external data. With the HASH interface, users can sift, select, browse, collate, investigate, download and visualise the entire currently known Galactic PNe diversity. HASH provides the community with the most complete and reliable data with which to undertake new science.
DescriptionSession II: Evolution of Planetary Nebulae
Persistent Identifierhttp://hdl.handle.net/10722/232761
ISSN
2023 SCImago Journal Rankings: 0.180
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorParker, QA-
dc.contributor.authorBojicic, IS-
dc.contributor.authorFrew, DJ-
dc.date.accessioned2016-09-20T05:32:08Z-
dc.date.available2016-09-20T05:32:08Z-
dc.date.issued2016-
dc.identifier.citation11th Pacific Rim Conference on Stellar Astrophysics: Physics and Chemistry of the Late Stages of Stellar Evolution, Hong Kong, PR China, 14–17 December 2015. In Journal of Physics: Conference Series, 2016, v. 728, article no. 032008-
dc.identifier.issn1742-6588-
dc.identifier.urihttp://hdl.handle.net/10722/232761-
dc.descriptionSession II: Evolution of Planetary Nebulae-
dc.description.abstractBy incorporating our major recent discoveries with re-measured and verified contents of existing catalogues we provide, for the first time, an accessible, reliable, on-line SQL database for essential, up-to date information for all known Galactic planetary nebulae (PNe). We have attempted to: i) reliably remove PN mimics/false ID's that have biased previous studies and ii) provide accurate positions, sizes, morphologies, multi-wavelength imagery and spectroscopy. We also provide a link to CDS/Vizier for the archival history of each object and other valuable links to external data. With the HASH interface, users can sift, select, browse, collate, investigate, download and visualise the entire currently known Galactic PNe diversity. HASH provides the community with the most complete and reliable data with which to undertake new science.-
dc.languageeng-
dc.publisherInstitute of Physics Publishing. The Journal's web site is located at http://www.iop.org/EJ/journal/conf-
dc.relation.ispartofJournal of Physics: Conference Series-
dc.rightsJournal of Physics: Conference Series. Copyright © Institute of Physics Publishing.-
dc.rightsThis work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.-
dc.titleHASH: the Hong Kong/AAO/Strasbourg Hα planetary nebula database-
dc.typeConference_Paper-
dc.identifier.emailParker, QA: physhead@hku.hk-
dc.identifier.emailBojicic, IS: ibojicic@hku.hk-
dc.identifier.emailFrew, DJ: djfrew@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.authorityBojicic, IS=rp02020-
dc.identifier.authorityFrew, DJ=rp02013-
dc.description.naturepublished_or_final_version-
dc.identifier.doi10.1088/1742-6596/728/3/032008-
dc.identifier.scopuseid_2-s2.0-84989350521-
dc.identifier.hkuros266102-
dc.identifier.volume728, article no. 032008-
dc.identifier.spage032008-
dc.identifier.epage032008-
dc.identifier.isiWOS:000397958000017-
dc.publisher.placeUnited Kingdom-
dc.identifier.issnl1742-6588-

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