activity
20132023
most citedThe PdBI Arcsecond Whirlpool Survey (PAWS): Environmental Dependence of Giant Molecular Cloud Properties in M51

265 citations · 3.8k across the 60 of their papers we have counts for

collaborators
Showing 2020Show all

6 papers · 1 filter

astro-ph.GA2020★ 101 cited

The SEDIGISM survey: first data release and overview of the Galactic structure

F. Schuller, J. S. Urquhart, T. Csengeri +57

The SEDIGISM (Structure, Excitation and Dynamics of the Inner Galactic Interstellar Medium) survey used the APEX telescope to map 84 deg^2 of the Galactic plane between l = -60 deg…

astro-ph.GA2020★ 67 cited

The SEDIGISM survey: Molecular clouds in the inner Galaxy

A. Duarte-Cabral, D. Colombo, J. S. Urquhart +57

We use the 13CO(2-1) emission from the SEDIGISM high-resolution spectral-line survey of the inner Galaxy, to extract the molecular cloud population with a large dynamic range in sp…

astro-ph.GA2020★ 54 cited

The EDGE-CALIFA survey: exploring the role of the molecular gas on the galaxy star formation quenching

D. Colombo, S. F. Sanchez, A. D. Bolatto +11

Understanding how galaxies cease to form stars represents an outstanding challenge for galaxy evolution theories. This process of "star formation quenching" has been related to var…

astro-ph.GA2020★ 29 cited

How do different spiral arm models impact the ISM and GMC population?

Alex R. Pettitt, Clare L. Dobbs, Junichi Baba +4

The nature of galactic spiral arms in disc galaxies remains elusive. Regardless of the spiral model, arms are expected to play a role in sculpting the star-forming interstellar med…

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★ 9 cited

An imaging line survey of OMC-1 to OMC-3

N. Brinkmann, F. Wyrowski, J. Kauffmann +4

Aims: Our aim is to identify the dominant molecular cooling lines and characteristic emission features in the 1.3 mm window of distinct regions in the northern part of the Orion A…