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researcher

C. Ceccarelli

4 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author2

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph1
ORCID 0000-0001-9664-6292
same name
  • C. Ceccarelli — 175 papers, h 55
  • C. Ceccarelli — 57 papers, h 30
  • C. Ceccarelli — 51 papers, h 18
  • C. Ceccarelli — 15 papers, h 7
  • C. Ceccarelli — 1 paper, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20052025
most citedDeuterated H3+​ in proto-planetary disks

64 citations · 135 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2025★ 2 cited

Gas-phase formation routes of dimethyl sulfide in the interstellar medium

Gabriella Di Genova, Nadia Balucani, Luca Mancini +3

Context: Dimethyl sulfide (DMS; CH3​SCH3​) is an organosulfur compound that has been suggested as a potential biosignature in exoplanetary atmospheres. In addition to its tenta…

astro-ph.GA2010★ 16 cited

Herschel observations of deuterated water towards Sgr B2(M)

Claudia Comito, Peter Schilke, Rainer Rolffs +53

Observations of HDO are an important complement for studies of water, because they give strong constraints on the formation processes -- grain surfaces versus energetic process in…

astro-ph.GA2010★ 53 cited

Herschel observations of extra-ordinary sources: Detection of Hydrogen Fluoride in absorption towards Orion~KL

T. G. Phillips, E. A. Bergin, D. C. Lis +52

We report a detection of the fundamental rotational transition of hydrogen fluoride in absorption towards Orion KL using Herschel/HIFI. After the removal of contaminating features…

astro-ph2005★ 64 cited

Deuterated H3+​ in proto-planetary disks

Cecilia Ceccarelli, Carsten Dominik

Probing the gas and dust in proto-planetary disks is central for understanding the process of planet formation. In disks surrounding solar type protostars, the bulk of the disk mas…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.