Gas rotation curves in simulated high-redshift galaxies underestimate dynamical mass by up to 40% unless turbulent pressure support and non-spherical potentials are corrected.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Measuring dynamical masses from gas kinematics in simulated high-redshift galaxies
Gas rotation curves in simulated high-redshift galaxies underestimate dynamical mass by up to 40% unless turbulent pressure support and non-spherical potentials are corrected.