362 citations · 5.3k across the 126 of their papers we have counts for
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ATLASGAL-selected massive clumps in the inner Galaxy III. Dust Continuum Characterization of an Evolutionary Sample
C. König, J. S. Urquhart, T. Csengeri +8
The ATLASGAL survey provides an ideal basis for detailed studies of large numbers of massive star forming clumps covering the whole range of evolutionary stages. The ATLASGAL Top10…
Hot methanol from the inner region of the HH 212 protostellar system
S. Leurini, C. Codella, S. Cabrit +9
The mechanisms leading to the formation of disks around young stellar objects (YSOs) and to the launching of the associated jets are crucial to the understanding of the earliest st…
ATLASGAL -- A Galaxy-wide sample of dense filamentary structures
Guang-Xing Li, J. S. Urquhart, S. Leurini +4
[Abridged] Aims. We study the properties of filamentary structures from the ATLASGAL survey. Methods. We use the DisPerSE algorithm to identify spatially coherent structures locate…
Physical characteristics of bright Class I methanol masers
S. Leurini, K. M. Menten, C. M. Walmsley
Class I CHOH masers trace interstellar shocks. They have received little attention mostly as a consequence of their low luminosities; this situation has changed recently and Cl…
The rate and latency of star formation in dense, massive clumps in the Milky Way
M. Heyer, R. Gutermuth, J. S. Urquhart +5
Newborn stars form within the localized, high density regions of molecular clouds. The sequence and rate at which stars form in dense clumps and the dependence on local and global…
Observations and modelling of CO and [CI] in disks. First detections of [CI] and constraints on the carbon abundance
M. Kama, S. Bruderer, M. Carney +23
The gas-solid budget of carbon in protoplanetary disks is related to the composition of the cores and atmospheres of the planets forming in them. The key gas-phase carbon carriers…