activity
20072021
most citedThe formation of ethylene glycol and other complex organic molecules in star-forming regions

121 citations · 1.2k across the 32 of their papers we have counts for

collaborators
Showing 2018Show all

9 papers · 1 filter

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.SR2018★ 64 cited

Chasing discs around O-type (proto)stars - ALMA evidence for an SiO disc and disc wind from G17.64+0.16

L. T. Maud, R. Cesaroni, M. S. N. Kumar +28

We present high angular resolution 0.2 arcsec continuum and molecular emission line Atacama Large Millimeter/sub-millimeter Array (ALMA) observations of G17.64+0.16 in Band 6 (220G…

astro-ph.SR2018★ 13 cited

The SOMA Radio Survey. I. Comprehensive SEDs Of High-Mass Protostars From Infrared To Radio And The Emergence Of Ionization Feedback

V. Rosero, K. E. I. Tanaka, J. C. Tan +5

We study centimeter continuum emission of eight high- and intermediate-mass protostars that are part of the SOFIA Massive (SOMA) Star Formation Survey, thus building extended spect…

astro-ph.SR2018

Detecting Infall in High-Mass Protostellar Objects

Maria T. Beltrán, Qizhou Zhang, Víctor M. Rivilla

The role of accretion disks in the formation of low-mass stars has been well assessed by means of high angular resolution observations at various wavelengths. These findings confir…

astro-ph.SR2018★ 3 cited

Complex Organic Molecules in Hot Molecular Cores/Corinos: Physics and Chemistry

Maria T. Beltrán, Víctor M. Rivilla

Hot molecular cores (HMCs), the cradles of massive stars, are the most chemically rich sources in the Galaxy. The typical masses of these cores (few hundreds of solar masses) make…

astro-ph.SR2018★ 56 cited

Nitrogen fractionation in high-mass star-forming cores across the Galaxy

L. Colzi, F. Fontani, V. M. Rivilla +4

The fractionation of nitrogen (N) in star-forming regions is a poorly understood process. To put more stringent observational constraints on the N-fractionation, we have observed w…