Please use this identifier to cite or link to this item: http://hdl.handle.net/2080/2283
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dc.contributor.authorPradhan, A C-
dc.contributor.authorParthasarathy, M-
dc.contributor.authorMurthy, J-
dc.contributor.authorOjha, D K-
dc.date.accessioned2015-04-02T03:32:33Z-
dc.date.available2015-04-02T03:32:33Z-
dc.date.issued2015-02-
dc.identifier.citation33rd Meeting of Astronomical Society of India, at NCRA-TIFR, Pune, India, February 17 - 20, 2015en_US
dc.identifier.urihttp://hdl.handle.net/2080/2283-
dc.descriptionCopyright belongs to proceeding publisheren_US
dc.description.abstractWe present the first ultraviolet (UV) photometric observations of planetary nebulae (PNe) using observations made by Galaxy Evolution Explorer (GALEX). We found about 112 PNe observed by GALEX. We have determined the angular diameter of PNe in NUV and also in FUV for whichever source detection exists considering a 3¾ emission level above the background. Of the PNe, 20% are elliptical, 7% are bipolar and rest are circular in UV. The emission lines contributing to GALEX FUV flux are strong OV, C IV, and He II while the emission line contributing to the NUV flux are C III] and He II.en_US
dc.language.isoenen_US
dc.subjectultraviolet (UV)en_US
dc.subjectplanetary nebulae (PNe)en_US
dc.subjectGalaxy Evolution Explorer (GALEX)en_US
dc.subjectGALEX FUVen_US
dc.titleThe GALEX Observations of Planetary Nebulaeen_US
dc.typePresentationen_US
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