362 citations · 6.1k across the 101 of their papers we have counts for
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The Rosetta Stone project. III. ALMA synthetic observations of fragmentation in high-mass star-forming clumps
Alice Nucara, Alessio Traficante, Ugo Lebreuilly +23
The physical mechanisms that regulate the collapse of high-mass parsec-scale clumps and allow them to form clusters of new stars represent a crucial aspect of star formation. To in…
Near-Infrared Polarization from Unresolved Disks Around Brown Dwarfs and Young Stellar Objects
Dan P. Clemens, Thushara G. S. Pillai, Anneliese M. Rilinger +1
Wide-field near-infrared (NIR) polarimetry was used to examine disk systems around two brown dwarfs (BD) and two young stellar objects (YSO) embedded in the Heiles Cloud 2 (HCl2) d…
Discovery of a sub-Keplerian disk with jet around a 20Msun young star. ALMA observations of G023.01-00.41
A. Sanna, A. Koelligan, L. Moscadelli +9
It is well established that Solar-mass stars gain mass via disk accretion, until the mass reservoir of the disk is exhausted and dispersed, or condenses into planetesimals. Accreti…
TADPOL: A 1.3 mm Survey of Dust Polarization in Star-forming Cores and Regions
Charles L. H. Hull, Richard L. Plambeck, Woojin Kwon +22
We present λ1.3 mm CARMA observations of dust polarization toward 30 star-forming cores and 8 star-forming regions from the TADPOL survey. We show maps of all sources, and compare…
Misalignment of Magnetic Fields and Outflows in Protostellar Cores
Charles L. H. Hull, Richard L. Plambeck, Alberto D. Bolatto +22
We present results of 1.3 mm dust polarization observations toward 16 nearby, low-mass protostars, mapped with ~2.5" resolution at CARMA. The results show that magnetic fields in p…
Is protostellar heating sufficient to halt fragmentation? A case study of the massive protocluster G8.68-0.37
Steven N. Longmore, Thushara Pillai, Eric Keto +2
If star formation proceeds by thermal fragmentation and the subsequent gravitational collapse of the individual fragments, how is it possible to form fragments massive enough for O…