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...
Wedi'i Gadw mewn:
| Prif Awduron: | , , |
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| Fformat: | Artigo |
| Iaith: | Inglês |
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ITB Journal Publisher
2024-01-01
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| Cyfres: | Journal of Mathematical and Fundamental Sciences |
| Pynciau: | |
| Mynediad Ar-lein: | https://journals.itb.ac.id/index.php/jmfs/article/view/21621 |
| Tagiau: |
Dim Tagiau, Byddwch y cyntaf i dagio'r cofnod hwn!
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