Cold gas disks in main-sequence galaxies at cosmic noon: Low turbulence, flat rotation curves, and disk-halo degeneracy
Federico Lelli(Arcetri Astrophysical Observatory), Stacy McGaugh(Case Western Reserve University), Antonino Marasco(Osservatorio Astronomico di Padova), Zhi-Yu Zhang(Nanjing University), Enrico M. Di Teodoro(Australian National University), James M. Schombert(Willamette University), Lingrui Lin(Nanjing University), P. P. Papadopoulos(Aristotle University of Thessaloniki), Thomas G. Bisbas(University of Cologne)
Cited by 42
Related Papers
The EAGLE simulations: atomic hydrogen associated with galaxies
|Monthly Notices of the Royal Astronomical Society|2016|161
Off the Baryonic Tully–Fisher Relation: A Population of Baryon-dominated Ultra-diffuse Galaxies
|The Astrophysical Journal Letters|2019|143
Non-circular motions and the diversity of dwarf galaxy rotation curves
|Monthly Notices of the Royal Astronomical Society|2018|139
MAGNUM survey: Compact jets causing large turmoil in galaxies
|Astronomy and Astrophysics|2021|139
The environmental dependence of H i in galaxies in the eagle simulations
|Monthly Notices of the Royal Astronomical Society|2016|104