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Article: Orientation of Galactic Bulge Planetary Nebulae toward the Galactic Center

TitleOrientation of Galactic Bulge Planetary Nebulae toward the Galactic Center
Authors
Danehkar, AParker, QA
KeywordsAstrophysics - Astrophysics of Galaxies
Issue Date2016
Citation
Proceedings of the International Astronomical Union, 2016, v. 10, p. 128-130 How to Cite?
DOI: http://dx.doi.org/10.1017/S1743921315007681
AbstractWe have used the Wide Field Spectrograph on the Australian National University 2.3-m telescope to perform the integral field spectroscopy for a sample of the Galactic planetary nebulae. The spatially resolved velocity distributions of the H$\alpha$ emission line were used to determine the kinematic features and nebular orientations. Our findings show that some bulge planetary nebulae toward the Galactic center have a particular orientation.
Persistent Identifierhttp://hdl.handle.net/10722/211194
ISI Accession Number ID
WOS:000452768300030

 

DC FieldValueLanguage
dc.contributor.authorDanehkar, A-
dc.contributor.authorParker, QA-
dc.date.accessioned2015-07-08T03:22:52Z-
dc.date.available2015-07-08T03:22:52Z-
dc.date.issued2016-
dc.identifier.citationProceedings of the International Astronomical Union, 2016, v. 10, p. 128-130-
dc.identifier.urihttp://hdl.handle.net/10722/211194-
dc.description.abstractWe have used the Wide Field Spectrograph on the Australian National University 2.3-m telescope to perform the integral field spectroscopy for a sample of the Galactic planetary nebulae. The spatially resolved velocity distributions of the H$\alpha$ emission line were used to determine the kinematic features and nebular orientations. Our findings show that some bulge planetary nebulae toward the Galactic center have a particular orientation.-
dc.languageeng-
dc.relation.ispartofProceedings of the International Astronomical Union-
dc.subjectAstrophysics - Astrophysics of Galaxies-
dc.titleOrientation of Galactic Bulge Planetary Nebulae toward the Galactic Center-
dc.typeArticle-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.description.naturepostprint-
dc.identifier.doi10.1017/S1743921315007681-
dc.identifier.volume10-
dc.identifier.spage128-
dc.identifier.epage130-
dc.identifier.isiWOS:000452768300030-

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