601 citations · 4k across the 61 of their papers we have counts for
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Dust hot spots at 10 au scales around the Class 0 binary IRAS 16293-2422 A: a departure from the passive irradiation model
M. J. Maureira, M. Gong, J. E. Pineda +6
Characterizing the physical conditions at disk scales in Class 0 sources is crucial for constraining the protostellar accretion process and the initial conditions for planet format…
The Central 1000 au of a Pre-stellar Core Revealed with ALMA. II. Almost Complete Freeze-out
Paola Caselli, Jaime E. Pineda, Olli Sipilä +18
Pre-stellar cores represent the initial conditions in the process of star and planet formation. Their low temperatures (10 K) allow the formation of thick icy dust mantles, whic…
Gas flow and accretion via spiral streamers and circumstellar disks in a young binary protostar
Felipe O. Alves, Paola Caselli, Josep M. Girart +4
The majority of stars are part of gravitationally bound stellar systems, such as binaries. Observations of protobinary systems constrain the conditions that lead to stellar multipl…
Evolution of complex organic molecules in hot molecular cores: Synthetic spectra at (sub-)mm wavebands
Rumpa Choudhury, Peter Schilke, Gwendoline Stéphan +4
Hot molecular cores (HMCs) are intermediate stages of high-mass star formation and are also known for their rich emission line spectra at (sub-)mm wavebands. The observed spectral…
Gas-phase CO depletion and N2H+ abundances in starless cores
N. Lippok, R. Launhardt, D. Semenov +10
Seven isolated, nearby low-mass starless molecular cloud cores have been observed as part of the Herschel key program Earliest Phases of Star formation (EPoS). By applying a ray-tr…
Dusty OB stars in the Small Magellanic Cloud - II: Extragalactic Disks or Examples of the Pleiades Phenomenon?
Joshua J. Adams, Joshua D. Simon, Alberto D. Bolatto +6
We use mid-infrared Spitzer spectroscopy and far-infrared Herschel photometry for a sample of twenty main sequence O9--B2 stars in the Small Magellanic Cloud (SMC) with strong 24 m…