activity
20062020
most citedThe photodissociation and chemistry of CO isotopologues: applications to interstellar clouds and circumstellar disks

551 citations · 6.3k across the 71 of their papers we have counts for

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Showing 2013Show all

14 papers · 1 filter

astro-ph.SR2013★ 122 cited

A recent accretion burst in the low-mass protostar IRAS 15398-3359: ALMA imaging of its related chemistry

Jes K. Jorgensen, Ruud Visser, Nami Sakai +8

Low-mass protostars have been suggested to show highly variable accretion rates through-out their evolution. Such changes in accretion, and related heating of their ambient envelop…

astro-ph.GA2013★ 48 cited

Deuterated water in the solar-type protostars NGC 1333 IRAS 4A and IRAS 4B

A. Coutens, C. Vastel, S. Cabrit +19

Aims. The aim of this paper is to study deuterated water in the solar-type protostars NGC1333 IRAS4A and IRAS4B, to compare their HDO abundance distribution with other star-forming…

astro-ph.SR2013★ 58 cited

Radionuclide Ionization in Protoplanetary Disks: Calculations of Decay Product Radiative Transfer

L. Ilsedore Cleeves, Fred C. Adams, Edwin A. Bergin +1

We present simple analytic solutions for the ionization rate arising from the decay of short-lived radionuclides (SLRs) within protoplanetary disks. We solve the rad…

astro-ph.GA2013★ 42 cited

Waterfalls around protostars: Infall motions towards Class 0/I envelopes as probed by water

J. C. Mottram, E. F. van Dishoeck, M. Schmalzl +4

Abridged abstract: For stars to form, material must fall inwards from core scales through the envelope towards the central protostar. The velocity profile around protostars is poor…

astro-ph.SR2013★ 70 cited

Deep observations of O2 toward a low-mass protostar with Herschel-HIFI

Umut A. Yıldız, Kinsuk Acharyya, Paul F. Goldsmith +13

According to traditional gas-phase chemical models, O2 should be abundant in molecular clouds, but until recently, attempts to detect interstellar O2 line emission with ground- and…

astro-ph.SR2013★ 43 cited

Observational evidence for dissociative shocks in the inner 100 AU of low-mass protostars using Herschel-HIFI

L. E. Kristensen, E. F. van Dishoeck, A. O. Benz +3

Herschel-HIFI spectra of H2O towards low-mass protostars show a distinct velocity component not seen in observations from the ground of CO or other species. The aim is to character…