activity
20152023
most citedPHANGS CO kinematics: disk orientations and rotation curves at 150 pc resolution

156 citations · 961 across the 16 of their papers we have counts for

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Showing astro-ph.GAShow all

24 papers · 1 filter

astro-ph.GA20231 cited

The EDGE-CALIFA Survey: Spatially Resolved 13CO(1-0) Observations and Variations in 12CO(1-0)/13CO(1-0) in Nearby Galaxies on kpc Scales

Yixian Cao, Tony Wong, Alberto D. Bolatto +12

We present 13CO(1-0) observations for the EDGE-CALIFA survey, which is a mapping survey of 126 nearby galaxies at a typical spatial resolution of 1.5 kpc. Using detected 12CO(1-0)…

astro-ph.GA202245 cited

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

Si-Yue Yu, Veselina Kalinova, Dario Colombo +9

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 depende…

astro-ph.GA202214 cited

Which galaxy property is the best gauge of the oxygen abundance?

P. Alvarez-Hurtado, J. K. Barrera-Ballesteros, S. F. Sánchez +3

We present an extensive exploration of the impact of 29 physical parameters in the oxygen abundance for a sample of 299 star-forming galaxies extracted from the extended CALIFA sam…

astro-ph.GA202118 cited

High Resolution LAsMA CO and CO Observation of the G305 Giant Molecular Cloud Complex : I. Feedback on the Molecular Gas

P. Mazumdar, F. Wyrowski, D. Colombo +3

We observed the G305 star forming complex in the lines of CO and CO to investigate how molecular gas surrounding the central stellar clusters is being…

astro-ph.GA2021

The EDGE-CALIFA Survey: Central molecular gas depletion in AGN host galaxies -- a smoking gun for quenching?

Sara L. Ellison, Tony Wong, Sebastian F. Sanchez +8

Feedback from an active galactic nucleus (AGN) is often implicated as a mechanism that leads to the quenching of galactic star formation. However, AGN-driven quenching is challengi…

astro-ph.GA2021

Identification of prestellar cores in high-mass star forming clumps via observations with ALMA

E. Redaelli, S. Bovino, A. Giannetti +5

Context. The different theoretical models concerning the formation of high-mass stars make distinct predictions regarding their progenitors, i.e. the high-mass prestellar cores. Ho…