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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Bibliographic Details
Published in:Proceedings of the International Astronomical Union 2016-10, Vol.12 (S323), p.333-334
Main Authors: Aksaker, Nazim, Yerli, Sinan K., Kızıloğlu, Ümit, Atalay, Betül
Format: Article
Language:English
Subjects:
Astronomy
Contributed Papers
Emission
Emission standards
Fluxes
Northern Hemisphere
Photometry
Planetary nebulae
Spectrometry
Spectrophotometry
Standard data
Supernova remnants
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Summary: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.
ISSN:1743-9213
1743-9221
DOI:10.1017/S1743921317001909