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Formation of the Stellar System and the Central Gravitation-Potential Vessel of Galaxies

Published online by Cambridge University Press:  09 June 2023

Keiichi Kodaira Open the ORCID record for Keiichi Kodaira [Opens in a new window]  and
Veselina Kalinova
Keiichi Kodaira
Affiliation:
Max Planck Institute for Radioastronomy, Auf dem Hügel 69, 53121 Bonn, Germany email: kodaira_keiichi0815@soken.ac.jp National Astronomical Observatory of Japan, Osawa2-21-1, Mitaka-shi, Tokyo, Japan PC 181-8588 SOKENDAI, International Village Hayama-machi, Miura-gun, Kanagawa-ken, Japan, PC 240-0193
Veselina Kalinova
Affiliation:
Max Planck Institute for Radioastronomy, Auf dem Hügel 69, 53121 Bonn, Germany email: kodaira_keiichi0815@soken.ac.jp
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Abstract

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The formation of the global stellar system of galaxies are studied through the circular velocity curves of CALIFA nearby galaxies by sequencing the depth and size of the central gravitation-potential vessel and its dynamical mass, relative to the masses of the stellar system and of the parent halo, with the population or age parameters, to explore the dynamical characteristics of the dissipative contracting baryonic matter.

Keywords

galaxies: kinematics and dynamicsgalaxies: structuregalaxies: evolution
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 17 , Symposium S373: Resolving the Rise and Fall of Star Formation in Galaxies , August 2021 , pp. 128 - 131
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Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

References

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