activity
20022026
most citedThe Dynamics of Massive Starless Cores with ALMA

170 citations · 6.6k across the 187 of their papers we have counts for

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Showing 2018Show all

14 papers · 1 filter

astro-ph.GA2018★ 21 cited

Multicomponent kinematics in a massive filamentary IRDC

Vlas Sokolov, Ke Wang, Jaime E. Pineda +6

To probe the initial conditions for high-mass star and cluster formation, we investigate the properties of dense filaments within the infrared dark cloud G035.39-00.33 (IRDC G035.3…

astro-ph.GA2018★ 49 cited

First ALMA maps of HCO, an important precursor of complex organic molecules, towards IRAS 16293-2422

V. M. Rivilla, M. T. Beltrán, A. Vasyunin +4

The formyl radical HCO has been proposed as the basic precursor of many complex organic molecules such as methanol (CHOH) or glycolaldehyde (CHOHCHO). Using ALMA, we have m…

astro-ph.GA2018★ 18 cited

Protonated CO2 in massive star-forming clumps

F. Fontani, A. Vagnoli, M. Padovani +3

Interstellar CO2 is an important reservoir of carbon and oxygen, and one of the major constituents of the icy mantles of dust grains, but it is not observable directly in the cold…

astro-ph.GA2018★ 6 cited

The first detections of the key prebiotic molecule PO in star-forming regions

Víctor M. Rivilla, Francesco Fontani, Maite Beltrán +4

Phosphorus is a crucial element in prebiotic chemistry, especially the PO bond, which is key for the formation of the backbone of the deoxyribonucleic acid. So far, PO had only…

astro-ph.SR2018★ 114 cited

First Detection of the Simplest Organic Acid in a Protoplanetary Disk

Cécile Favre, Davide Fedele, Dmitry Semenov +14

The formation of asteroids, comets and planets occurs in the interior of protoplanetary disks during the early phase of star formation. Consequently, the chemical composition of th…

astro-ph.GA2018★ 57 cited

SOLIS IV. Hydrocarbons in the OMC-2 FIR 4 region, a probe of energetic particle irradiation of the region

C. Favre, C. Ceccarelli, A. López-Sepulcre +16

We report new interferometric images of cyclopropenylidene, c-CH, towards the young protocluster OMC-2 FIR\,4. The observations were performed at 82 and 85 GHz with the NOr…