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

Title Orientation of Galactic Bulge Planetary Nebulae toward the Galactic Center Danehkar, AParker, QA Astrophysics - Astrophysics of Galaxies 2014 ArXiv e-prints, 2014, v. 1412, p. 12-12 How to Cite? We 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. http://hdl.handle.net/10722/211194

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.issued2014-
dc.identifier.citationArXiv e-prints, 2014, v. 1412, p. 12-12-
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.ispartofArXiv e-prints-
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.volume1412-
dc.identifier.spage12-
dc.identifier.epage12-