Emission Lines of Northern Planetary Nebulae

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AKSAKER N., YERLİ S. K. , Kiziloglu U., Atalay B.

323RD Symposium of the International-Astronomical-Union (IAU), Beijing, China, 10 - 14 October 2016, vol.12, pp.333-334 identifier

  • Publication Type: Conference Paper / Full Text
  • Volume: 12
  • Doi Number: 10.1017/s1743921317001909
  • City: Beijing
  • Country: China
  • Page Numbers: pp.333-334


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.