Ionized and molecular gas kinematics in a z=1.4 star-forming galaxy

We present deep observations of a \(z=1.4\) massive, star-forming galaxy in molecular and ionized gas at comparable spatial resolution (CO 3-2, NOEMA; H\(\alpha\), LBT). The kinematic tracers agree well, indicating that both gas phases are subject to the same gravitational potential and physical pro...

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Veröffentlicht in:	arXiv.org 2018-02
Hauptverfasser:	Übler, Hannah D N, Genzel, Reinhard, Tacconi, Linda J, ster Schreiber, Natascha M, Neri, Roberto, Contursi, Alessandra, Belli, Sirio, Nelson, Erica J, Lang, Philipp, T Taro Shimizu, Davies, Ric, Herrera-Camus, Rodrigo, Lutz, Dieter, Plewa, Philipp M, Price, Sedona H, Schuster, Karl, Sternberg, Amiel, Tadaki, Ken-ichi, Wisnioski, Emily, Wuyts, Stijn
Format:	Artikel
Sprache:	eng
Schlagworte:	Baryons Bayesian analysis Dark matter Galaxies Gas dynamics Kinematics Molecular gases Physics - Astrophysics of Galaxies Spatial resolution Star formation Tracers Vapor phases
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