activity
20172023
most citedSulphur chemistry in the L1544 pre-stellar core

140 citations · 878 across the 19 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.GA2020★ 27 cited

Gas-phase Elemental abundances in Molecular cloudS (GEMS) III. Unlocking the CS chemistry: the CS+O reaction

N. Bulut, O. Roncero, A. Aguado +36

CS is among the most abundant gas-phase S-bearing molecules in cold dark molecular clouds. It is easily observable with several transitions in the millimeter wavelength range, and…

astro-ph.EP2020★ 9 cited

Visualizing the Kinematics of Planet Formation

Disk Dynamics Collaboration, Philip J. Armitage, Jaehan Bae +23

A stunning range of substructures in the dust of protoplanetary disks is routinely observed across a range of wavelengths. These gaps, rings and spirals are highly indicative of a…

astro-ph.IM2020★ 1 cited

A Prospective ISRO-CfA Himalayan Sub-millimeter-wave Observatory Initiative

T. K. Sridharan, Shmuel Bialy, Raymond Blundell +20

The Smithsonian Astrophysical Observatory (SAO), a member of the Center for Astrophysics | Harvard and Smithsonian, is in discussions with the Space Applications Centre (SAC) of th…

astro-ph.SR2020★ 17 cited

A 3mm chemical exploration of small organics in Class I YSOs

Romane Le Gal, Karin I. Öberg, Jane Huang +8

There is mounting evidence that the composition and structure of planetary systems are intimately linked to their birth environments. During the past decade, several spectral surve…

astro-ph.GA2020★ 82 cited

Gas phase Elemental abundances in Molecular cloudS (GEMS). II. On the quest for the sulphur reservoir in molecular clouds: the case

D. Navarro-Almaida, R. Le Gal, A. Fuente +30

Sulphur is one of the most abundant elements in the Universe. Surprisingly, sulphuretted molecules are not as abundant as expected in the interstellar medium, and the identity of t…

astro-ph.SR2020★ 69 cited

An ALMA Survey of HCO in Protoplanetary Disks

Jamila Pegues, Karin I. Öberg, Jennifer B. Bergner +13

HCO is one of the most abundant organic molecules in protoplanetary disks and can serve as a precursor to more complex organic chemistry. We present an ALMA survey of HCO t…