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20112026
most citedA protostellar system fed by a streamer of 10,500 au length

166 citations · 1.5k across the 32 of their papers we have counts for

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9 papers · 1 filter

astro-ph.GA2022★ 23 cited

Models of Rotating Infall for the B335 Protostar

Neal J. Evans, Yao-Lun Yang, Joel D. Green +7

Models of the protostellar source, B335, are developed using axisymmetric three-dimensional models to resolve conflicts found in one-dimensional models. The models are constrained…

astro-ph.GA2022★ 32 cited

FAUST III. Misaligned rotations of the envelope, outflow, and disks in the multiple protostellar system of VLA 16232417

Satoshi Ohashi, Claudio Codella, Nami Sakai +69

We report a study of the low-mass Class-0 multiple system VLA 1623AB in the Ophiuchus star-forming region, using HCO (), CS (), and CCH () lines as…

astro-ph.GA2021★ 43 cited

Accretion Flows or Outflow Cavities? Uncovering the Gas Dynamics around Lupus 3-MMS

Travis J. Thieme, Shih-Ping Lai, Sheng-Jun Lin +6

Understanding how material accretes onto the rotationally supported disk from the surrounding envelope of gas and dust in the youngest protostellar systems is important for describ…

astro-ph.GA2021★ 9 cited

No impact of core-scale magnetic field, turbulence, or velocity gradient on sizes of protostellar disks in Orion A

Hsi-Wei Yen, Bo Zhao, Patrick M. Koch +1

We compared the sizes and fluxes of a sample of protostellar disks in Orion A measured with the ALMA 0.87 mm continuum data from the VANDAM survey with the physical properties of t…

astro-ph.GA2020★ 166 cited

A protostellar system fed by a streamer of 10,500 au length

Jaime E. Pineda, Dominique Segura-Cox, Paola Caselli +5

Binary formation is an important aspect of star formation. One possible route for close-in binary formation is disk fragmentation. Recent observations show small scale…

astro-ph.GA2020★ 23 cited

Effect of grain size distribution and size-dependent grain heating on molecular abundances in starless and pre-stellar cores

O. Sipilä, B. Zhao, P. Caselli

We present a new gas-grain chemical model to constrain the effect of grain size distribution on molecular abundances in starless and pre-stellar cores. We introduce grain-size depe…

astro-ph.GA2020★ 37 cited

Rapid Elimination of Small Dust Grains in Molecular Clouds

Kedron Silsbee, Alexei Ivlev, Paola Caselli +2

We argue that impact velocities between dust grains with sizes less than in molecular cloud cores are dominated by drift arising from ambipolar diffusion. This effe…

astro-ph.GA2019★ 42 cited

The specific angular momentum radial profile in dense cores: improved initial conditions for disk formation

Jaime E. Pineda, Bo Zhao, Anika Schmiedeke +5

The determination of the specific angular momentum radial profile, , in the early stages of star formation is crucial to constrain star and circumstellar disk formation theor…

astro-ph.GA2018★ 48 cited

On the Effects of Self-Obscuration in the (Sub-)Millimeter Spectral Indices and Appearance of Protostellar Disks

Roberto Galván-Madrid, Hauyu Baobab Liu, Andrés F. Izquierdo +5

In this paper we explore the effects of self-obscuration in protostellar disks with a radially decreasing temperature gradient and a colder midplane. We are motivated by recent rep…