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Fragmentation in filamentary molecular clouds
Yanett Contreras, Guido Garay, Jill M. Rathborne +1
Recent surveys of dust continuum emission at sub-mm wavelengths have shown that filamentary molecular clouds are ubiquitous along the Galactic plane. These structures are inhomogen…
High-mass star-forming cloud G0.38+0.04 in the Galactic Center Dust Ridge contains H2CO and SiO masers
Adam Ginsburg, Andrew Walsh, Christian Henkel +15
We have discovered a new HCO (formaldehyde) 4.82966 GHz maser in Galactic Center Cloud C, G0.38+0.04. At the time of acceptance, this is the eighth region con…
Far-Infrared Dust Temperatures and Column Densities of the MALT90 Molecular Clump Sample
Andrés E. Guzmán, Patricio Sanhueza, Yanett Contreras +4
We present dust column densities and dust temperatures for young high-mass molecular clumps from the Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey, derived fro…
Tracing the Conversion of Gas into Stars in Young Massive Cluster Progenitors
D. L. Walker, S. N. Longmore, N. Bastian +5
Whilst young massive clusters (YMCs; 10 M, age 100 Myr) have been identified in significant numbers, their progenitor gas clouds have elude…
A cluster in the making: ALMA reveals the initial conditions for high-mass cluster formation
J. M. Rathborne, S. N. Longmore, J. M. Jackson +9
G0.253+0.016 is a molecular clump that appears to be on the verge of forming a high mass, Arches-like cluster. Here we present new ALMA observations of its small-scale (~0.07 pc) 3…