activity
20072025
most citedThe Effects of Radiative Transfer on Low-Mass Star Formation

313 citations · 1.8k across the 41 of their papers we have counts for

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Showing 2020Show all

14 papers · 1 filter

astro-ph.GA202033 cited

The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars IV. Unveiling the Embedded Intermediate-Mass Protostar and Disk within OMC2-FIR3/HOPS-370

John J. Tobin, Patrick Sheehan, Nickalas Reynolds +13

We present ALMA (0.87~mm and 1.3~mm) and VLA (9~mm) observations toward the candidate intermediate-mass protostar OMC2-FIR3 (HOPS-370; L~314~L) at 0.1" (40~…

astro-ph.GA2020

Application of Convolutional Neural Networks to Identify Protostellar Outflows in CO Emission

Duo Xu, Stella S. R. Offner, Robert Gutermuth +1

We adopt the deep learning method CASI-3D (Convolutional Approach to Structure Identification-3D) to identify protostellar outflows in molecular line spectra. We conduct magneto-hy…

astro-ph.GA2020

STARFORGE: The effects of protostellar outflows on the IMF

Dávid Guszejnov, Michael Y. Grudić, Philip F. Hopkins +2

The initial mass function (IMF) of stars is a key quantity affecting almost every field of astrophysics, yet it remains unclear what physical mechanisms determine it. We present th…

astro-ph.SR202018 cited

Aluminum-26 Enrichment in the Surface of Protostellar Disks Due to Protostellar Cosmic Rays

Brandt A. L. Gaches, Stefanie Walch, Stella S. R. Walch +1

The radioactive decay of aluminum-26 (Al) is an important heating source in early planet formation. Since its discovery, there have been several mechanisms proposed to intro…

astro-ph.GA202017 cited

Ubiquitous supersonic component in L1688 coherent cores

Spandan Choudhury, Jaime E. Pineda, Paola Caselli +15

Context : Star formation takes place in cold dense cores in molecular clouds. Earlier observations have found that dense cores exhibit subsonic non-thermal velocity dispersions. In…

astro-ph.SR202063 cited

Zooming in on Individual Star Formation: Low- and High-mass Stars

Anna L. Rosen, Stella S. R. Offner, Sarah I. Sadavoy +3

Star formation is a multi-scale, multi-physics problem ranging from the size scale of molecular clouds (10s pc) down to the size scales of dense prestellar cores (0.1 p…