Optical Spectroscopy and Photoionization Model of Planetary Nebula NGC 6572

We investigated NGC 6572 through optical spectroscopy to determine its kinematical and chemical properties. Two intermediate dispersion spectra (R~5000) centered around Hα and Hβ were used to derive the nebular expansion velocity from emission lines associated with Hα, Hβ, [OIII], [NII], and [SII] i...

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Bibliographic Details

Published in:	Journal of Mathematical and Fundamental Sciences
Main Authors:	Muhammad Fajrin, Hakim Luthfi Malasan, Evan Irawan Akbar
Format:	Article
Language:	English
Published:	ITB Journal Publisher 2024-01-01
Subjects:	chemical abundances expansion velocity photoionization model planetary nebula spectroscopy
Online Access:	https://journals.itb.ac.id/index.php/jmfs/article/view/21621