Electronic gas density in the Galaxy NGC 3310 with Pyneb

Authors

  • Adan Artola Universidad Nacional Autónoma de Honduras

DOI:

https://doi.org/10.5377/ce.v11i2.8677

Keywords:

NGC 3310, Spectroscopy, Line analysis, Equivalent Width, Flux

Abstract

In this document we present results of the analysis and reduction from the optical spectrum (λ3600 − λ7000 Å) of NGC 3310 starburst galaxy. The eletronic density analisys showed a value of ne = 167.85e−/cm3 for the studied region. We also compute flux and equivalent width for the strongest emisión and absortion lines that are present in the galaxy.

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Author Biography

Adan Artola, Universidad Nacional Autónoma de Honduras

Master en Astronomía y Astrofísica, Departamento de Astronomía y Astrofísica, Facultad de Ciencias Espaciales de la Universidad Nacional Autónoma de Honduras 

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Published

2019-11-01

How to Cite

Artola, A. (2019). Electronic gas density in the Galaxy NGC 3310 with Pyneb. Ciencias Espaciales, 11(2), 31–37. https://doi.org/10.5377/ce.v11i2.8677

Issue

Vol. 11 No. 2 (2018)

Section

Astronomy and Astrophysics