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 2021Show all

11 papers · 1 filter

cs.NE2021★ 8 cited

NEORL: NeuroEvolution Optimization with Reinforcement Learning

Majdi I. Radaideh, Katelin Du, Paul Seurin +4

We present an open-source Python framework for NeuroEvolution Optimization with Reinforcement Learning (NEORL) developed at the Massachusetts Institute of Technology. NEORL offers…

astro-ph.GA2021★ 30 cited

The SEDIGISM survey: a search for molecular outflows

A. Y. Yang, J. S. Urquhart, F. Wyrowski +19

Context. The formation processes of massive stars are still unclear but a picture is emerging involving accretion disks and molecular outflows in what appears to be a scaled-up ver…

astro-ph.GA2021★ 19 cited

OGHReS: Large-scale filaments in the outer Galaxy

D. Colombo, C. König, J. S. Urquhart +9

Filaments are a ubiquitous morphological feature of the molecular interstellar medium and are identified as sites of star formation. In recent years, more than 100 large-scale fila…

astro-ph.GA2021★ 17 cited

A Kpc Scale Molecular Wave in the Inner Galaxy: Feather of the Milky Way?

V. S. Veena, P. Schilke, Á. Sánchez-Monge +7

We report the discovery of a velocity coherent, kpc-scale molecular structure towards the Galactic center region with an angular extent of 30deg and an aspect ratio of 60:1. The ki…

astro-ph.GA2021★ 24 cited

The SEDIGISM survey: The influence of spiral arms on the molecular gas distribution of the inner Milky Way

D. Colombo, A. Duarte-Cabral, A. R. Pettitt +23

The morphology of the Milky Way is still a matter of debate. In order to shed light on uncertainties surrounding the structure of the Galaxy, in this paper, we study the imprint of…

astro-ph.GA2021★ 16 cited

The EDGE-CALIFA survey: The resolved star formation efficiency and local physical conditions

V. Villanueva, A. Bolatto, S. Vogel +14

We measure the star formation rate (SFR) per unit gas mass and the star formation efficiency (SFE for total gas, SFE for the molecular gas) in 81 nearby gal…