Please use this identifier to cite or link to this item: http://hdl.handle.net/2080/2691
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dc.contributor.authorPradhan, Ananta C-
dc.date.accessioned2017-03-30T18:05:35Z-
dc.date.available2017-03-30T18:05:35Z-
dc.date.issued2017-03-
dc.identifier.citation35th Annual Meeting of the Astronomical Society of India (ASI), BISR, Jaipur, India, 6-10 March 2017en_US
dc.identifier.urihttp://hdl.handle.net/2080/2691-
dc.description.abstractA planetary nebulae consists of a hot, luminous central star and an expanding glowing shell of gas and dust. The central star of most of the planetary nebulae (PNe) is a very hot object which is bright in ultraviolet (UV) and hence, UV observations explore the properties of these objects. We present the UV images of 108 PNe using observations made by Galaxy Evolution Explorer (GALEX). We have determined the angular diameter of PNe in NUV and also in FUV for whichever source detection exists considering a 3σ emission level above the background. We determine the morphology and many other physical parameters related to UV observations of PNe.en_US
dc.subjectPlanetary Nebulae.en_US
dc.subjectPlanetary Nebulaeen_US
dc.titleGalex Observations of Planetary Nebulaeen_US
dc.typePresentationen_US
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