Optical Spectroscopy and Photoionization Model of Planetary Nebula NGC 6572

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

Internet

https://journals.itb.ac.id/index.php/jmfs/article/view/21621

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