Neutral atomic and molecular gas dynamics in the nearby spiral galaxies NGC 1512, NGC 4535, and NGC 7496

Neutral atomic gas (HI) effectively traces galactic dynamics across mid to large galactocentric radii. However, its limitations in observing small-scale changes within the central few kiloparsecs, coupled with the often observed HI deficit in galactic centers, necessitates using molecular gas emissi...

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Veröffentlicht in:	arXiv.org 2024-07
Hauptverfasser:	Laudage, Sebastian, Eibensteiner, Cosima, Bigiel, Frank, Leroy, Adam K, Meidt, Sharon, Schinnerer, Eva, W J G de Blok, Querejeta, Miguele, Stuber, Sophia, Colombo, Dario, Rosolowsky, Erik, Pisano, D J, Dyas Utomo, Levy, Rebecca C, Klessen, Ralf, Cao, Yixian, Koch, Eric W, Kurapati, Sushma, Sanchez-Blazquez, Patricia, Neumann, Justus, Neumann, Lukas, Hsi-An Pan, Williams, Thomas G
Format:	Artikel
Sprache:	eng
Schlagworte:	Emissions Galactic evolution Gas dynamics Molecular gases Physics - Astrophysics of Galaxies Spiral galaxies
Online-Zugang:	Volltext
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