133 citations · 133 across the 1 of their papers we have counts for
7 papers
ALMA observations of envelopes around first hydrostatic core candidates
Maria Jose Maureira, Hector G. Arce, Michael M. Dunham +4
We present ALMA 3 mm molecular line and continuum observations with a resolution of ~3.5" towards five first hydrostatic core (FHSC) candidates (L1451-mm, Per-bolo 58, Per-bolo 45,…
Illuminating a tadpole's metamorphosis III: quantifying past and present environmental impact
Megan Reiter, Thomas J. Haworth, Andrés E. Guzmán +3
We combine MUSE and ALMA observations with theoretical models to evaluate how a tadpole-shaped globule located in the Carina Nebula has been influenced by its environment. This glo…
A ringed pole-on outflow from DO Tauri revealed by ALMA
M. Fernández López, L. A. Zapata, L. F. Rodríguez +3
We present new ALMA Band 6 observations including the CO(2-1) line and 1.3 mm continuum emission from the surroundings of the young stellar object DO Tauri. The ALMA CO molecular d…
The Interaction Between the Supernova Remnant W41 and the Filamentary Infrared Dark Cloud G23.33-0.30
Taylor G. Hogge, James M. Jackson, David Allingham +6
G23.33-0.30 is a 600 infrared dark molecular filament that exhibits large NH velocity dispersions () and bright, narrow NH(3,3) line…
An Asymmetric Keplerian Disk Surrounding the O-type Protostar IRAS165474247
Luis A. Zapata, Guido Garay, Aina Palau +4
During the last decades, a great interest has emerged to know if even the most massive stars in our galaxy (namely the spectral O-type stars) are formed in a similar manner as the…
G337.342-0.119 (the "Pebble"): A Cold, Dense, High-Mass Molecular Cloud with Unusually Large Linewidths and a Candidate High-Mass Star Cluster Progenitor
James M. Jackson, Yanett Contreras, Jill M. Rathborne +7
Exactly how high-mass star clusters form, especially the young massive clusters (YMCs: age Myr; mass solar masses), remains an open problem, largely because they are…