activity
20142016
most citedA cluster in the making: ALMA reveals the initial conditions for high-mass cluster formation

118 citations · 365 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA201650 cited

Characterizing the properties of cluster precursors in the MALT90 survey

Yanett Contreras, Jill M. Rathborne, Andres Guzman +4

In the Milky Way there are thousands of stellar clusters each harboring from a hundred to a million stars. Although clusters are common, the initial conditions of cluster formation…

astro-ph.GA2015118 cited

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…

astro-ph.GA2014108 cited

IN-SYNC II: Virial Stars from Sub-Virial Cores -- The Velocity Dispersion of Embedded Pre-Main-Sequence Stars in NGC 1333

Jonathan B. Foster, Michiel Cottaar, Kevin R. Covey +14

The initial velocity dispersion of newborn stars is a major unconstrained aspect of star formation theory. Using near-infrared spectra obtained with the APOGEE spectrograph, we sho…

astro-ph.SR201426 cited

ALMA Observations of the IRDC Clump G34.43+00.24 MM3: 278 GHz Class I Methanol Masers

Takahiro Yanagida, Takeshi Sakai, Tomoya Hirota +7

We have observed a molecular clump (MM3) associated with the infrared dark cloud G34.43+00.24 in the CH3OH J_K=9_{-1}--8_0 E, 5_0-4_0 E, and 5_{-1}-4_{-1} E lines at sub-arcsecond…

astro-ph.GA201419 cited

Absorption Filaments Towards the Massive Clump G0.253+0.016

John Bally, J. M. Rathborne, S. N. Longmore +11

ALMA HCO+ observations of the infrared dark cloud G0.253+0.016 located in the Central Molecular Zone of the Galaxy are presented. The 89 GHz emission is area-filling, optically thi…

astro-ph.GA201444 cited

Distributed Low-Mass Star Formation in the IRDC G34.43+00.24

Jonathan B. Foster, Héctor G. Arce, Marc Kassis +9

We have used deep near-infrared observations with adaptive optics to discover a distributed population of low-mass protostars within the filamentary Infrared Dark Cloud G34.43+00.2…