activity
20052023
most citedGravity or turbulence? -III. Evidence of pure thermal Jeans fragmentation at ~0.1 pc scale

116 citations · 703 across the 22 of their papers we have counts for

collaborators

20 papers

astro-ph.GA2023★ 9 cited

Infall and Outflow Towards High-mass Starless Clump Candidates

T. G. S. Pillai, J. S. Urquhart, S. Leurini +6

The evolutionary sequence for high-mass star formation starts with massive starless clumps that go on to form protostellar, young stellar objects and then compact HII regions. Whil…

astro-ph.GA2022★ 8 cited

The initial conditions for young massive cluster formation in the Galactic Centre: convergence of large-scale gas flows

Bethan A. Williams, Daniel L. Walker, Steven N. Longmore +12

Young massive clusters (YMCs) are compact (1 pc), high-mass (>10 M) stellar systems of significant scientific interest. Due to their rarity and rapid fo…

astro-ph.GA2021

Discovery of a Highly Collimated Flow from the High-Mass Protostar ISOSS J23053+5953 SMM2

T. M., Rodríguez, P. Hofner +7

We present Very Large Array C, X, and Q-band continuum observations, as well as 1.3 mm continuum and CO(2-1) observations with the Submillimeter Array toward the high-mass protoste…

astro-ph.GA2021★ 39 cited

Star formation in 'the Brick': ALMA reveals an active proto-cluster in the Galactic centre cloud G0.253+0.016

Daniel L. Walker, Steven N. Longmore, John Bally +16

G0.253+0.016, aka 'the Brick', is one of the most massive (> 10^5 Msun) and dense (> 10^4 cm-3) molecular clouds in the Milky Way's Central Molecular Zone. Previous observations ha…

astro-ph.IM2021★ 2 cited

Offline Correction of Atmospheric Effects on Single-Dish Radio Spectroscopy

Tsuyoshi Sawada, Chin-Shin Chang, Harold Francke +8

We present a method to mitigate the atmospheric effects (residual atmospheric lines) in single-dish radio spectroscopy caused by the elevation difference between the target and ref…

astro-ph.IM2021★ 2 cited

Towards the processing, review, and delivery of 80% of the ALMA data by the Joint ALMA Observatory (JAO)

Jorge F. García Yus, Bill Dent, Drew Brisbin +3

After eight observing Cycles, the Atacama Large Millimeter-submillimeter Array (ALMA) is capable of observing in eight different bands (covering a frequency range from 84 to 950 GH…