261 citations · 2.6k across the 62 of their papers we have counts for
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The SVS13-A Class I chemical complexity as revealed by S-bearing species. SOLIS XIII
C. Codella, E. Bianchi, L. Podio +13
Aims: The goal is to obtain a census of S-bearing species using interferometric images, towards SVS13-A, a Class I object associated with a hot corino rich in interstellar complex…
Theoretical computations on the efficiency of acetaldehyde formation on interstellar icy grains
Joan Enrique-Romero, Cecilia Ceccarelli, Albert Rimola +3
Interstellar grains are known to be important actors in the formation of interstellar molecules such as H, water, ammonia, and methanol. It has been suggested that the so-calle…
Structures and Properties of Known and Postulated Interstellar Cations
Lorenzo Tinacci, Stefano Pantaleone, Andrea Maranzana +3
Positive ions play a fundamental role in the interstellar chemistry, especially in cold environments where chemistry is believed to be mainly ion-driven. However, in contrast with…
ORion Alma New GEneration Survey (ORANGES) I. Dust continuum and free-free emission of OMC-2/3 filament protostars
M. Bouvier, A. López-Sepulcre, C. Ceccarelli +3
The spectral energy distribution (SED) in the millimetre (mm) to centimetre (cm) range is a useful tool for characterising the dust in protostellar envelopes as well as free-free e…
Rotating Motion of the Outflow of IRAS 16293-2422 A1 at its Origin Point near the Protostar
Yoko Oya, Yoshimasa Watanabe, Ana López-Sepulcre +4
The Class 0 protostar IRAS 162932422 Source A is known to be a binary system (A1 and A2) or even a multiple system, which processes a complex outflow structure. We have observed…
H2 formation on interstellar grains and the fate of reaction energy
Stefano Pantaleone, Joan Enrique-Romero, Cecilia Ceccarelli +4
Molecular hydrogen is the most abundant molecular species in the Universe. While no doubts exist that it is mainly formed on the interstellar dust grain surfaces, many details of t…