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S. Molinari

113 papers hereh-index 4911.4k citations354 works total

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

author position
  • first author12
  • middle author67
  • last author17

Across the 96 of 113 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA69
  • astro-ph17
  • astro-ph.SR13
  • astro-ph.IM8
  • astro-ph.EP3
  • astro-ph.HE1
same name
  • S. Molinari — 24 papers, h 5
  • S. Molinari — 23 papers, h 0
  • S. Molinari — 19 papers, h 6
  • S. Molinari — 17 papers, h 8
  • S. Molinari — 14 papers
  • S. Molinari — 11 papers, h 23

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
19982023
most citedCharacterizing interstellar filaments with Herschel in IC5146

792 citations · 7.8k across the 112 of their papers we have counts for

collaborators
Showing 2001Show all

3 papers · 1 filter

astro-ph2001★ 27 cited

Far Infrared Spectroscopy of the HH 1/2 Outflow

Sergio Molinari, Alberto Noriega-Crespo

The HH 1/2 system has been observed with the two spectrometers on board the Infrared Space Observatory. Diffuse [CII] 158um emission indicate the presence of a Photo-Dissociation R…

astro-ph2001★ 56 cited

A molecular-line study of clumps with embedded high-mass protostar candidates

J. Brand, R. Cesaroni, F. Palla +1

We present molecular line observations made with the IRAM 30-m telescope of the immediate surroundings of a sample of 11 candidate high-mass protostars. These observations are part…

astro-ph2001★ 41 cited

Infrared and Millimetric Study of the Young Outflow Cepheus E

A. Moro-Martin, A. Noriega-Crespo, S. Molinari +3

The Cepheus E outflow has been studied in the mid and far infrared using the ISO CAM and LWS instruments, and at millimetric wavelengths using OVRO. In the near and mid-IR, its mor…

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