activity
20132026
most citedThe lifecycle of molecular clouds in nearby star-forming disc galaxies

292 citations · 7.2k across the 143 of their papers we have counts for

collaborators
Showing 2020Show all

13 papers · 1 filter

astro-ph.GA2020★ 19 cited

Galaxies within galaxies in the TIMER survey: stellar populations of inner bars are scaled replicas of main bars

Adrian Bittner, Adriana de Lorenzo-Cáceres, Dimitri A. Gadotti +11

Inner bars are frequent structures in the local Universe and thought to substantially influence the nuclear regions of disc galaxies. In this study we explore the structure and dyn…

astro-ph.GA2020★ 202 cited

Distances to PHANGS Galaxies: New Tip of the Red Giant Branch Measurements and Adopted Distances

Gagandeep S. Anand, Janice C. Lee, Schuyler D. Van Dyk +29

PHANGS-HST is an ultraviolet-optical imaging survey of 38 spiral galaxies within ~20 Mpc. Combined with the PHANGS-ALMA, PHANGS-MUSE surveys and other multiwavelength data, the dat…

astro-ph.GA2020★ 97 cited

On the duration of the embedded phase of star formation

Jaeyeon Kim, Mélanie Chevance, J. M. Diederik Kruijssen +23

Feedback from massive stars plays a key role in molecular cloud evolution. After the onset of star formation, the young stellar population is exposed by photoionization, winds, sup…

astro-ph.GA2020★ 15 cited

ALMA Resolves Giant Molecular Clouds in a Tidal Dwarf Galaxy

M. Querejeta, F. Lelli, E. Schinnerer +12

Tidal dwarf galaxies (TDGs) are gravitationally bound condensations of gas and stars formed during galaxy interactions. Here we present multi-configuration ALMA observations of J10…

astro-ph.GA2020★ 12 cited

The kinematics of young and old stellar populations in nuclear rings of MUSE TIMER galaxies

D. Rosado-Belza, J. Falcón-Barroso, J. H. Knapen +12

Studying the stellar kinematics of galaxies is a key tool in the reconstruction of their evolution. However, the current measurements of the stellar kinematics are complicated by s…

astro-ph.GA2020★ 11 cited

Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies

Mélanie Chevance, J. M. Diederik Kruijssen, Mark R. Krumholz +28

It is a major open question which physical processes stop the accretion of gas onto giant molecular clouds (GMCs) and limit the efficiency at which gas is converted into stars with…

astro-ph.GA2020★ 85 cited

The inside-out formation of nuclear discs and the absence of old central spheroids in barred galaxies of the TIMER survey

Adrian Bittner, Patricia Sánchez-Blázquez, Dimitri A. Gadotti +13

The centres of disc galaxies host a variety of structures built via both internal and external processes. In this study, we constrain the formation and evolution of these central s…

astro-ph.GA2020★ 104 cited

Kinematic signatures of nuclear discs and bar-driven secular evolution in nearby galaxies of the MUSE TIMER project

Dimitri A. Gadotti, Adrian Bittner, Jesus Falcon-Barroso +13

The central regions of disc galaxies hold clues to the processes that dominate their formation and evolution. The TIMER project has obtained high signal-to-noise and spatial resolu…

astro-ph.GA2020★ 153 cited

Molecular Gas Properties on Cloud Scales Across the Local Star-forming Galaxy Population

Jiayi Sun, Adam K. Leroy, Eva Schinnerer +34

Using the PHANGS-ALMA CO (2-1) survey, we characterize molecular gas properties on 100 pc scales across 102,778 independent sightlines in 70 nearby galaxies. This yields th…

astro-ph.GA2020★ 156 cited

PHANGS CO kinematics: disk orientations and rotation curves at 150 pc resolution

Philipp Lang, Sharon E. Meidt, Erik Rosolowsky +24

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 measurem…

astro-ph.GA2020★ 146 cited

Dynamical Equilibrium in the Molecular ISM in 28 Nearby Star-Forming Galaxies

Jiayi Sun, Adam K. Leroy, Eve C. Ostriker +26

We compare the observed turbulent pressure in molecular gas, , to the required pressure for the interstellar gas to stay in equilibrium in the gravitational potent…

astro-ph.GA2020

Pa, H, and Attenuation in NGC 5194 and NGC 6946

Sarah Kessler, Adam Leroy, Miguel Querejeta +5

We combine Hubble Space Telescope (HST) Paschen (Pa) imaging with ground-based, previously published H maps to estimate the attenuation affecting H, A(H), across th…

astro-ph.GA2020★ 38 cited

A model for the onset of self-gravitation and star formation in molecular gas governed by galactic forces: II. the bottleneck to collapse set by cloud-environment decoupling

Sharon E. Meidt, Simon C. O. Glover, J. M. Diederik Kruijssen +12

In Meidt et al. (2018), we showed that gas kinematics on the scale of individual molecular clouds are not dominated by self-gravity but also track a component that originates with…