activity
20192025
most citedComparing the pre-SNe feedback and environmental pressures for 6000 HII regions across 19 nearby spiral galaxies

55 citations · 246 across the 12 of their papers we have counts for

collaborators
Showing 2021Show all

7 papers · 1 filter

astro-ph.GA202155 cited

Comparing the pre-SNe feedback and environmental pressures for 6000 HII regions across 19 nearby spiral galaxies

A. T. Barnes, S. C. O. Glover, K. Kreckel +28

The feedback from young stars (i.e. pre-supernova) is thought to play a crucial role in molecular cloud destruction. In this paper, we assess the feedback mechanisms acting within…

astro-ph.GA202150 cited

Star Cluster Classification in the PHANGS-HST Survey: Comparison between Human and Machine Learning Approaches

Bradley C. Whitmore, Janice C. Lee, Rupali Chandar +21

When completed, the PHANGS-HST project will provide a census of roughly 50,000 compact star clusters and associations, as well as human morphological classifications for roughly 20…

astro-ph.IM2021

PHANGS-ALMA Data Processing and Pipeline

Adam K. Leroy, Annie Hughes, Daizhong Liu +65

We describe the processing of the PHANGS-ALMA survey and present the PHANGS-ALMA pipeline, a public software package that processes calibrated interferometric and total power data…

astro-ph.GA2021

Star formation scaling relations at ~100 pc from PHANGS: Impact of completeness and spatial scale

I. Pessa, E. Schinnerer, F. Belfiore +31

Aims: The complexity of star formation at the physical scale of molecular clouds is not yet fully understood. We investigate the mechanisms regulating the formation of stars in dif…

astro-ph.GA2021

The organization of cloud-scale gas density structure: high resolution CO vs. 3.6 m brightness contrasts in nearby galaxies

Sharon E. Meidt, Adam K. Leroy, Miguel Querejeta +29

In this paper we examine the factors that shape the distribution of molecular gas surface densities on the 150 pc scale across 67 morphologically diverse star-forming galaxies in t…

astro-ph.GA202137 cited

Applying the Tremaine-Weinberg Method to Nearby Galaxies: Stellar Mass-Based Pattern Speeds, and Comparisons with ISM Kinematics

Thomas G. Williams, Eva Schinnerer, Eric Emsellem +22

We apply the Tremaine-Weinberg method to 19 nearby galaxies using stellar mass surface densities and velocities derived from the PHANGS-MUSE survey, to calculate (primarily bar) pa…