PHANGS CO kinematics: disk orientations and rotation curves at 150 pc resolution
Author
dc.contributor.author
Lang, Philipp
Author
dc.contributor.author
Meidt, Sharon E.
Author
dc.contributor.author
Rosolowsky, Erik
Author
dc.contributor.author
Nofech, Joseph
Author
dc.contributor.author
Schinnerer, Eva
Author
dc.contributor.author
Leroy, Adam K.
Author
dc.contributor.author
Emsellem, Eric
Author
dc.contributor.author
Pessa, Ismael
Author
dc.contributor.author
Glover, Simon C.O.
Author
dc.contributor.author
Groves, Brent
Author
dc.contributor.author
Hughes, Anne
Author
dc.contributor.author
Kruijssen, J. M. Diederik
Author
dc.contributor.author
Querejeta, Miguel
Author
dc.contributor.author
Schruba, Andreas
Author
dc.contributor.author
Bigiel, Frank
Author
dc.contributor.author
Blanc Mendiberri, Guillermo
Author
dc.contributor.author
Chevance, Mélanie
Author
dc.contributor.author
Colombo, Dario
Author
dc.contributor.author
Faesi, Christopher
Author
dc.contributor.author
Henshaw, Jonathan D.
Author
dc.contributor.author
Herrera, Cinthya N.
Author
dc.contributor.author
Liu, Daizhong
Author
dc.contributor.author
Pety, Jérôme
Author
dc.contributor.author
Puschnig, Johannes
Author
dc.contributor.author
Saito, Toshiki
Author
dc.contributor.author
Sun, Jiayi
Author
dc.contributor.author
Usero, Antonio
Admission date
dc.date.accessioned
2020-10-06T21:35:27Z
Available date
dc.date.available
2020-10-06T21:35:27Z
Publication date
dc.date.issued
2020
Cita de ítem
dc.identifier.citation
The Astrophysical Journal 897(2):122
es_ES
Identifier
dc.identifier.other
10.3847/1538-4357/ab9953
Identifier
dc.identifier.uri
https://repositorio.uchile.cl/handle/2250/177013
Abstract
dc.description.abstract
We present kinematic orientations and high-resolution (150 pc) rotation curves for 67 main-sequence star-forming galaxies surveyed in CO (2-1) emission by PHANGS-ALMA. Our measurements are based on the application of a new fitting method tailored to CO velocity fields. Our approach identifies an optimal global orientation as a way to reduce the impact of nonaxisymmetric (bar and spiral) features and the uneven spatial sampling characteristic of CO emission in the inner regions of nearby galaxies. The method performs especially well when applied to the large number of independent lines of sight contained in the PHANGS CO velocity fields mapped at 1 '' resolution. The high-resolution rotation curves fitted to these data are sensitive probes of mass distribution in the inner regions of these galaxies. We use the inner slope as well as the amplitude of our fitted rotation curves to demonstrate that CO is a reliable global dynamical mass tracer. From the consistency between photometric orientations from the literature and kinematic orientations determined with our method, we infer that the shapes of stellar disks in the mass range of log(M-star (M-circle dot)) = 9.0-10.9 probed by our sample are very close to circular and have uniform thickness.
es_ES
Patrocinador
dc.description.sponsorship
European Research Council (ERC)
694343
Natural Sciences and Engineering Research Council of Canada
RGPIN-201703987
German Research Foundation (DFG)
KR4801/1-1
German Research Foundation (DFG)
KR4801/2-1
European Research Council (ERC)
714907
German Research Foundation (DFG)
SFB 881
138713538
EXC 2181/1-390900948
Programme National "Physique et Chimie du Milieu Interstellaire" (PCMI) of CNRS/INSU
INC/INP - CEA
Centre National D'etudes Spatiales
Programme National Cosmology and Galaxies (PNCG) of CNRS/INSU
INP
IN2P3
French Atomic Energy Commission
European Union's Horizon 2020 research and innovation program
726384