Warped Disk Galaxies. I. Linking U type Warps in Groups/Clusters to Jellyfish Galaxies

Warped Disk Galaxies. I. Linking U type Warps in Groups/Clusters to Jellyfish Galaxies

arped disk galaxies are classified into two morphologies: S- and U-types. Conventional theories routinely attribute both types to galactic tidal interaction and/or gas accretion, but reproducing of U-types in simulations is extremely challenging. Here we investigate whether both types are governed b...

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Veröffentlicht in:arXiv.org 2022-08
Hauptverfasser: Zee, Woong-Bae G, Suk-Jin, Yoon, Jun-Sung, Moon, Sung-Ho, An, Paudel, Sanjaya, Kiyun Yun
Format: Artikel
Sprache:eng
Schlagworte:
Accretion disks
Deposition
Disk galaxies
Galactic clusters
Galaxy distribution
Physics - Astrophysics of Galaxies
Ram pressure
Star & galaxy formation
Star formation rate
Stellar mass
Tidal effects
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Zusammenfassung:arped disk galaxies are classified into two morphologies: S- and U-types. Conventional theories routinely attribute both types to galactic tidal interaction and/or gas accretion, but reproducing of U-types in simulations is extremely challenging. Here we investigate whether both types are governed by the same mechanisms using the most extensive sample of \(\sim\)8000 nearby (0.02\,\(
ISSN:2331-8422
DOI:10.48550/arxiv.2208.05534