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Emission Lines of Northern Planetary Nebulae
In this work, we present results of long slit spectrophotometric emission line flux observations of selected planetary nebulae (PNe). We have measured absolute fluxes and equivalent widths (EW) of all observable emission lines. In addition to these observations, electron temperatures (Te), densities...
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Published in: | Proceedings of the International Astronomical Union 2016-10, Vol.12 (S323), p.333-334 |
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creator | Aksaker, Nazim Yerli, Sinan K. Kızıloğlu, Ümit Atalay, Betül |
description | In this work, we present results of long slit spectrophotometric emission line flux observations of selected planetary nebulae (PNe). We have measured absolute fluxes and equivalent widths (EW) of all observable emission lines. In addition to these observations, electron temperatures (Te), densities (Ne), and chemical abundances were also calculated. The main purpose of this work is to fill the gaps in emission line flux standards for the northern hemisphere. It is expected that the measured fluxes would be used as standard data set for further photometric and spectrometric measurements of HII regions, supernova remnants etc. |
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subjects | Astronomy Contributed Papers Emission Emission standards Fluxes Northern Hemisphere Photometry Planetary nebulae Spectrometry Spectrophotometry Standard data Supernova remnants |
title | Emission Lines of Northern Planetary Nebulae |
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