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 2014Show all

10 papers · 1 filter

astro-ph.EP2014★ 5 cited

Complex organic molecules in protostellar environments in the SKA era

C. Codella, L. Podio, F. Fontani +10

Molecular complexity builds up at each step of the Sun-like star formation process, starting from simple molecules and ending up in large polyatomic species. Complex organic molecu…

astro-ph.EP2014★ 59 cited

Astrochemistry at work in the L1157-B1 shock: acetaldehyde formation

C. Codella, F. Fontani, C. Ceccarelli +5

The formation of complex organic molecules (COMs) in protostellar environments is a hotly debated topic. In particular, the relative importance of the gas phase processes as compar…

astro-ph.SR2014★ 82 cited

Deuteration and evolution in the massive star formation process: the role of surface chemistry

F. Fontani, G. Busquet, Aina Palau +5

An ever growing number of observational and theoretical evidence suggests that the deuterated fraction (column density ratio between a species containing D and its hydrogenated cou…

astro-ph.GA2014★ 122 cited

ATLASGAL-selected massive clumps in the inner Galaxy: I. CO depletion and isotopic ratios

A. Giannetti, F. Wyrowski, J. Brand +8

In the low-mass regime, it is found that the gas-phase abundances of C-bearing molecules in cold starless cores rapidly decrease with increasing density, as the molecules form mant…

astro-ph.SR2014★ 35 cited

A high resolution study of complex organic molecules in hot cores

Hannah Calcutt, Serena Viti, Claudio Codella +3

We present the results of a line identification analysis using data from the IRAM Plateau de Bure Inferferometer, focusing on six massive star-forming hot cores: G31.41+0.31, G29.9…

astro-ph.SR2014★ 150 cited

The dynamical properties of dense filaments in the infrared dark cloud G035.39-00.33

Jonathan D. Henshaw, Paola Caselli, Francesco Fontani +2

Infrared Dark Clouds (IRDCs) are unique laboratories to study the initial conditions of high-mass star and star cluster formation. We present high-sensitivity and high-angular reso…