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Conference Paper: A Preferred Orientation Angle for Bipolar Planetary Nebulae

TitleA Preferred Orientation Angle for Bipolar Planetary Nebulae
Authors
Ritter, AParker, QA
Keywordsmethods: statistical
astronomical data bases
planetary nebulae: general
Issue Date2020
PublisherMDPI AG. The Journal's web site is located at http://www.mdpi.com/journal/galaxies
Citation
Workplans II: Workshop for Planetary Nebula Observations, Leiden, Netherlands, 16–20 December 2019. In Galaxies, 2020, v. 8 n. 2, p. article no. 34:1-6 How to Cite?
DOI: http://dx.doi.org/10.3390/galaxies8020034
AbstractWe present preliminary results from measuring Galactic orientation angles of 766 elliptical and bipolar Planetary Nebulae (PNe) in the Hong Kong/Australian Astronomical Observatory/Strasbourg Observatory H-alpha Planetary Nebula research platform and database (HASH DB). For elliptical PNe the distribution of orientation angles is found to be more or less uniform. However, for bipolar PNe there is statistically significant evidence for preferred orientation angles (as tentatively reported before with smaller samples) across the whole Galaxy.
Persistent Identifierhttp://hdl.handle.net/10722/283001
ISSN
2075-4434
2020 SCImago Journal Rankings: 0.646
ISI Accession Number ID
WOS:000551227500021

 

DC FieldValueLanguage
dc.contributor.authorRitter, A-
dc.contributor.authorParker, QA-
dc.date.accessioned2020-06-05T06:23:55Z-
dc.date.available2020-06-05T06:23:55Z-
dc.date.issued2020-
dc.identifier.citationWorkplans II: Workshop for Planetary Nebula Observations, Leiden, Netherlands, 16–20 December 2019. In Galaxies, 2020, v. 8 n. 2, p. article no. 34:1-6-
dc.identifier.issn2075-4434-
dc.identifier.urihttp://hdl.handle.net/10722/283001-
dc.description.abstractWe present preliminary results from measuring Galactic orientation angles of 766 elliptical and bipolar Planetary Nebulae (PNe) in the Hong Kong/Australian Astronomical Observatory/Strasbourg Observatory H-alpha Planetary Nebula research platform and database (HASH DB). For elliptical PNe the distribution of orientation angles is found to be more or less uniform. However, for bipolar PNe there is statistically significant evidence for preferred orientation angles (as tentatively reported before with smaller samples) across the whole Galaxy.-
dc.languageeng-
dc.publisherMDPI AG. The Journal's web site is located at http://www.mdpi.com/journal/galaxies-
dc.relation.ispartofGalaxies-
dc.relation.ispartofWorkPLANS II: Workshop for Planetary Nebula Observations-
dc.rightsThis work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.-
dc.subjectmethods: statistical-
dc.subjectastronomical data bases-
dc.subjectplanetary nebulae: general-
dc.titleA Preferred Orientation Angle for Bipolar Planetary Nebulae-
dc.typeConference_Paper-
dc.identifier.emailRitter, A: aritter@hku.hk-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.description.naturepublished_or_final_version-
dc.identifier.doi10.3390/galaxies8020034-
dc.identifier.scopuseid_2-s2.0-85084647697-
dc.identifier.hkuros309989-
dc.identifier.volume8-
dc.identifier.issue2-
dc.identifier.isiWOS:000551227500021-
dc.publisher.placeSwitzerland-
dc.identifier.issnl2075-4434-

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