Spectrum evaluation of the Planetary Nebula NGC 1501

Authors

  • Eduardo Enrique Rodas-Quito Universidad Nacional Autónoma de Honduras
  • Hugo Hugo Ramos-Hernández Universidad Nacional Autónoma de Honduras

DOI:

https://doi.org/10.5377/ce.v11i2.8676

Keywords:

Spectroscopy, Planetary Nebula, Stellar Evolution

Abstract

The spectrum analysis of the nebula designated in the New General Catalog with number 1501 (NGC1501) was performed, using the Image Reduction and Analysis Facility (IRAF) software as an analysis tool, with which several treatments were carried out to the spectrum of the object aforementioned. The reference star used for the NGC1501 spectrum calibration is G191B2B. As a final result, data on some of the elements present in the nebula, an estimation of the quantity of interstellar dust in the line of sight Earth-nebula, electronic density of the nebula and electronic temperature of the gas that makes up the nebula were obtained.

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Author Biographies

Eduardo Enrique Rodas-Quito, Universidad Nacional Autónoma de Honduras

Máster en Astronomía y Astrofísica, Departamento de Arqueoastronomía y Astronomía Cultural, Facultad de Ciencias Espaciales, de la Universidad Nacional Autónoma de Honduras 

Hugo Hugo Ramos-Hernández, Universidad Nacional Autónoma de Honduras

Ingeniero Industrial, Departamento de Astronomía y Astrofísica, Facultad de Ciencias Espaciales  de la Uiversidad Nacional Autónoma de Honduras

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Published

2019-11-01

How to Cite

Rodas-Quito, E. E., & Ramos-Hernández, H. H. (2019). Spectrum evaluation of the Planetary Nebula NGC 1501. Ciencias Espaciales, 11(2), 38–56. https://doi.org/10.5377/ce.v11i2.8676

Issue

Vol. 11 No. 2 (2018)

Section

Astronomy and Astrophysics