Study of The Parameters of Star Forming Regions in The Galaxy NGC 628

We present a study of star-forming regions in the galaxy NGC 628 using near and mid infrared data from the JWST telescope, the CO line (2 − 1) by the ALMA radio interferometer, and the Hα, Hβ, and OIII lines by the MUSE spectrograph. The star formation regions were taken from the works of Kongiu and Groves.

Authors

К. И. Смирнова (ORCID: https://orcid.org/0000-0002-3102-6663)
D. S. Wiebe

Institutions

Ural Federal University (RU)
Institute of Astronomy (RU)

Publication Details

Published: 2025-01-01
DOI: https://doi.org/10.15826/b978-5-7996-3986-0.74
Primary Topic: Stellar, planetary, and galactic studies
Type: article
Field-Weighted Citation Impact: 0.00

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article

Study of The Parameters of Star Forming Regions in The Galaxy NGC 628

К. И. Смирнова, D. S. Wiebe

Jan 1, 2025

1 links

Stellar, planetary, and galactic studies

article

Study of The Parameters of Star Forming Regions in The Galaxy NGC 628

К. И. Смирнова, D. S. Wiebe

January 1, 2025article en

Abstract

Ural Federal University (RU), Institute of Astronomy (RU)

Openalex Percentile: Top 87%

Stellar, planetary, and galactic studies

DOI Open Access PDF OpenAlex

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Study of The Parameters of Star Forming Regions in The Galaxy NGC 628 — К. И. Смирнова, D. S. Wiebe · (2025) | TGRS Research Map | TGRS