activity
19972026
most citedWater in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results

262 citations · 10.6k across the 258 of their papers we have counts for

collaborators
Showing 2014Show all

16 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.GA2014★ 25 cited

Fast molecular jet from L1157-mm

M. Tafalla, R. Bachiller, B. Lefloch +4

L1157-mm powers a molecular outflow that is well-known for its shock-induced chemical activity in several hot-spots. We have studied the molecular emission toward L1157-mm searchin…

astro-ph.GA2014★ 37 cited

The density structure of the L1157 molecular outflow

A. I. Gómez-Ruiz, C. Codella, B. Lefloch +6

We present a multiline CS survey towards the brightest bow-shock B1 in the prototypical chemically active protostellar outflow L1157. We made use of (sub-)mm data obtained in the f…

astro-ph.GA2014★ 31 cited

SiO excitation from dense shocks in the earliest stages of massive star formation

S. Leurini, C. Codella, A. López-Sepulcre +3

Molecular outflows are a direct consequence of accretion, and therefore they represent one of the best tracers of accretion processes in the still poorly understood early phases of…

astro-ph.GA2014★ 15 cited

First spectrally-resolved H observations towards HH 54 / Low HO abundance in shocks

G. Santangelo, S. Antoniucci, B. Nisini +11

Context: Herschel observations suggest that the HO distribution in outflows from low-mass stars resembles the H emission. It is still unclear which of the different excitat…