activity
20042023
most citedSubmm line imaging of Orion-KL with the Submillimeter Array

120 citations · 1.7k across the 42 of their papers we have counts for

collaborators

42 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.GA2023★ 30 cited

Mother of Dragons: A Massive, quiescent core in the dragon cloud (IRDC G028.37+00.07)

A. T. Barnes, J. Liu, Q. Zhang +15

Context: Core accretion models of massive star formation require the existence of massive, starless cores within molecular clouds. Yet, only a small number of candidates for such t…

astro-ph.GA2021★ 7 cited

Orientation effect on the ligh curve shape of periodic methanol maser sources

J. Morgan, D. J. van der Walt, J. O. Chibueze +1

We report the results of our pilot millimeter observations of periodic maser sources. Using SMA, we carried out 1.3\,mm observations of G22.3570.066 and G25.4110.105, while A…

astro-ph.GA2021★ 42 cited

Magnetic Fields in Massive Star-Forming Regions (MagMaR) I. Linear Polarized Imaging of the UCHII Region G5.89-0.39

M. Fernández-López, P. Sanhueza, L. A. Zapata +14

We report 1.2 mm polarized continuum emission observations carried out with the Atacama Large Millimeter/submillimeter Array (ALMA) toward the high-mass star formation region G5.89…

astro-ph.GA2021★ 7 cited

The physical and chemical structure of high-mass star-forming regions. Unraveling chemical complexity with the NOEMA large program "CORE"

C. Gieser, H. Beuther, D. Semenov +30

We use sub-arcsecond resolution (0.4) observations with NOEMA at 1.37 mm to study the dust emission and molecular gas of 18 high-mass star-forming regions. We combine the…

astro-ph.GA2020★ 29 cited

The role of the magnetic field in the fragmentation process: the case of G14.225-0.506

N. Añez-López, G. Busquet, P. M. Koch +8

B-fields are predicted to play a role in the formation of filamentary structures and their fragmentation process. We aim at investigating the role of the B-field in the process of…