activity
20202026
most citedFAUST I. The hot corino at the heart of the prototypical Class I protostar L1551 IRS5

51 citations · 337 across the 16 of their papers we have counts for

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Showing astro-ph.GAShow all

11 papers · 1 filter

astro-ph.GA2025

The Green Bank Ammonia Survey: Data Release 2

Jaime E. Pineda, Rachel K. Friesen, Erik Rosolowsky +22

We present an overview of the final data release (DR2) from the Green Bank Ammonia Survey (GAS). GAS is a Large Program at the Green Bank Telescope to map all Gould Belt star-formi…

astro-ph.GA2025★ 3 cited

Asymmetric accretion through a streamer onto the pre-stellar core H-MM1

Spandan Choudhury, Jongsoo Kim, Paola Caselli +2

CONTEXT: Dense cores are thought to be isolated from the surrounding cloud. However, observations of streamers and subsonic material outside core boundaries challenges this idea. A…

astro-ph.GA2023

Infall of material onto the filaments in Barnard 5

Spandan Choudhury, Jaime E. Pineda, Paola Caselli +3

Aims. We aim to study the structure and kinematics of the two filaments inside the subsonic core Barnard 5 in Perseus using high-resolution ( 2400 au) NH3 data and a multi…

astro-ph.GA2023★ 28 cited

Flow of gas detected from beyond the filaments to protostellar scales in Barnard 5

M. T. Valdivia-Mena, J. E. Pineda, D. M. Segura-Cox +7

The infall of gas from outside natal cores has proven to feed protostars after the main accretion phase (Class 0). This changes our view of star formation to a picture that include…

astro-ph.GA2022★ 7 cited

Velocity-Coherent Substructure in TMC-1: Inflow and Fragmentation

Simon E. T. Smith, Rachel Friesen, Antoine Marchal +11

Filamentary structures have been found nearly ubiquitously in molecular clouds and yet their formation and evolution is still poorly understood. We examine a segment of Taurus Mole…

astro-ph.GA2022★ 35 cited

An Interferometric View of H-MM1. I. Direct Observation of NH3 Depletion

Jaime E. Pineda, Jorma Harju, Paola Caselli +14

Spectral lines of ammonia, NH, are useful probes of the physical conditions in dense molecular cloud cores. In addition to advantages in spectroscopy, ammonia has also been sug…

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★ 25 cited

Are massive dense clumps truly sub-virial? A new analysis using Gould Belt ammonia data

Ayushi Singh, Christopher D. Matzner, Rachel K. Friesen +21

Dynamical studies of dense structures within molecular clouds often conclude that the most massive clumps contain too little kinetic energy for virial equilibrium, unless they are…

astro-ph.GA2021★ 25 cited

Transition from Coherent Cores to Surrounding Cloud in L1688

Spandan Choudhury, Jaime E. Pineda, Paola Caselli +8

Stars form in cold dense cores showing subsonic velocity dispersions. The parental molecular clouds display higher temperatures and supersonic velocity dispersions. The transition…

astro-ph.GA2020★ 17 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.GA2020★ 41 cited

Turbulence, Coherence and Collapse: Three Phases for Core Evolution

Stella S. R. Offner, Josh Taylor, Carleen Markey +6

We study the formation, evolution and collapse of dense cores by tracking structures in a magnetohydrodynamic simulation of a star-forming cloud. We identify cores using the dendro…