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20002023
most citedLarge-Scale Structure of the Molecular Gas in Taurus Revealed by High Linear Dynamic Range Spectral Line Mapping

486 citations · 7.9k across the 158 of their papers we have counts for

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Showing 2020Show all

13 papers · 1 filter

astro-ph.GA2020★ 27 cited

ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Detection of extremely high density compact structure of prestellar cores and multiple substructures within

Dipen Sahu, Sheng-Yuan Liu, Tie Liu +38

Prestellar cores are self-gravitating dense and cold structures within molecular clouds where future stars are born. They are expected, at the stage of transitioning to the protost…

astro-ph.GA2020★ 51 cited

ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP) II. Survey overview: a first look at 1.3 mm continuum maps and molecular outflows

Somnath Dutta, Chin-Fei Lee, Tie Liu +32

Planck Galactic Cold Clumps (PGCCs) are contemplated to be the ideal targets to probe the early phases of star formation. We have conducted a survey of 72 young dense cores inside…

astro-ph.IM2020

Applications of Machine Learning Algorithms In Processing Terahertz Spectroscopic Data

Young Min Seo, Paul F. Goldsmith, Volker Tolls +5

We present the data reduction software and the distribution of Level 1 and Level 2 products of the Stratospheric Terahertz Observatory 2 (STO2). STO2, a balloon-borne Terahertz tel…

astro-ph.GA2020★ 18 cited

Atomic and molecular gas properties during cloud formation

J. Syed, Y. Wang, H. Beuther +15

Molecular clouds, which harbor the birthplaces of stars, form out of the atomic phase of the interstellar medium (ISM). We aim to characterize the atomic and molecular phases of th…

astro-ph.GA2020★ 9 cited

A SOFIA Survey of [CII] in the galaxy M51 II. [CII] and CO kinematics across spiral arms

Jorge L. Pineda, Juergen Stutzki, Christof Buchbender +10

We present the first complete, velocity-resolved [CII] 158um image of the M51 grand-design spiral galaxy, observed with the upGREAT instrument on SOFIA. [CII] is an important trace…

astro-ph.GA2020★ 17 cited

HAWC+ Far-Infrared Observations of the Magnetic Field Geometry in M51 and NGC 891

Terry Jay Jones, Jin-Ah Kim, C. Darren Dowell +29

SOFIA HAWC+ polarimetry at $154~\micron$ is reported for the face-on galaxy M51 and the edge-on galaxy NGC 891. For M51, the polarization vectors generally follow the spiral patter…