The EDGE-CALIFA survey: The role of spiral arms and bars in driving central molecular gas concentrations

Shocks and torques produced by non-axisymmetric structures such as spiral arms and bars may transport gas to galaxy central regions. We test this hypothesis by studying the dependence of the concentration of CO luminosity ( C CO ) and molecular gas ( C mol ) and the star formation rate ( C SFR ) in...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2022-10, Vol.666, p.A175
Hauptverfasser:	Yu, Si-Yue, Kalinova, Veselina, Colombo, Dario, Bolatto, Alberto D., Wong, Tony, Levy, Rebecca C., Villanueva, Vicente, Sánchez, Sebastián F., Ho, Luis C., Vogel, Stuart N., Teuben, Peter, Rubio, Mónica
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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