Emission Lines of Northern Planetary Nebulae

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2016-10-14

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AKSAKER, NAZIM
Yerli, Sinan Kaan
Kiziloglu, Umit
Atalay, Betul

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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.

Subject Keywords

Planetary nebulae: general, Techniques: image processing, Techniques: spectroscopic

URI

https://hdl.handle.net/11511/35389

DOI

https://doi.org/10.1017/s1743921317001909

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Department of Physics, Conference / Seminar

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Citation Formats

N. AKSAKER, S. K. Yerli, U. Kiziloglu, and B. Atalay, “Emission Lines of Northern Planetary Nebulae,” 2016, vol. 12, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/35389.