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20012025
most citedAstronomical identification of CN-, the smallest observed molecular anion

244 citations · 4.4k across the 59 of their papers we have counts for

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Showing astro-ph.GAShow all

34 papers · 1 filter

astro-ph.GA2022★ 32 cited

FAUST III. Misaligned rotations of the envelope, outflow, and disks in the multiple protostellar system of VLA 16232417

Satoshi Ohashi, Claudio Codella, Nami Sakai +69

We report a study of the low-mass Class-0 multiple system VLA 1623AB in the Ophiuchus star-forming region, using HCO (), CS (), and CCH () lines as…

astro-ph.GA2020★ 22 cited

Hunting for hot corinos and WCCC sources in the OMC-2/3 filament

M. Bouvier, A. López-Sepulcre, C. Ceccarelli +5

Context: Solar-like protostars are known to be chemically rich, but it is not yet clear how much their chemical composition can vary and why. So far, two chemically distinct types…

astro-ph.GA2019★ 14 cited

Molecules in the CepE-mm jet: evidence for shock-driven photochemistry?

J. Ospina-Zamudio, B. Lefloch, C. Favre +6

The chemical composition of protostellar jets and its origin are still badly understood. More observational constraints are needed to make progress. With that objective, we have ca…

astro-ph.GA2019★ 40 cited

Interferometric observations of warm deuterated methanol in the inner regions of low-mass protostars

Vianney Taquet, Eleonora Bianchi, Claudio Codella +7

Methanol is a key species in astrochemistry since it is the most abundant organic molecule in the ISM and is thought to be the mother molecule of many complex organic species. Esti…

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…

astro-ph.GA2018★ 136 cited

Astrochemical evolution along star formation: Overview of the IRAM Large Program ASAI

B. Lefloch, R. Bachiller, C. Ceccarelli +27

Evidence is mounting that the small bodies of our Solar System, such as comets and asteroids, have at least partially inherited their chemical composition from the first phases of…