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M. Padovani

18 papers hereh-index 4112 citations19 works total

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

author position
  • middle author13
  • last author3

Across the 16 of 18 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA15
  • astro-ph.SR2
  • astro-ph.HE1
same name
  • M. Padovani — 84 papers, h 38
  • M. Padovani — 16 papers, h 4
  • M. Padovani — 4 papers
  • M. Padovani — 4 papers, h 3
  • M. Padovani — 2 papers, h 1
  • M. Padovani — 1 paper

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
20182026
most citedPhysical Processes in Star Formation

80 citations · 191 across the 17 of their papers we have counts for

collaborators
Showing 2024Show all

4 papers · 1 filter

astro-ph.GA2024★ 10 cited

A new analytic approach to infer the cosmic-ray ionization rate in hot molecular cores from HCO+, N2​H+, and CO observations

Gan Luo, Thomas G. Bisbas, Marco Padovani +1

The cosmic-ray ionization rate (ζ2​) is one of the key parameters in star formation, since it regulates the chemical and dynamical evolution of molecular clouds by ionizing molec…

astro-ph.GA2024

Astrochemistry on Galactic scales

L. Colzi, V. M. Rivilla, M. T. Beltrán +3

The increasing number of observations towards different environments in the Milky Way, as well as theoretical and experimental works, are improving our knowledge of the astrochemic…

astro-ph.GA2024★ 13 cited

Parsec-scale cosmic-ray ionisation rate in Orion

A. Socci, G. Sabatini, M. Padovani +2

Cosmic rays regulate the dynamics and the chemical processes in the densest and coldest regions of the ISM. Still, the determination of the cosmic-ray ionisation rate of H2​ (${ζ…

astro-ph.GA2024

Deciphering the Hidden Structures of HH 216 and Pillar IV in M16: Results from JWST and HST

L. K. Dewangan, O. R. Jadhav, A. K. Maity +6

To probe the star formation process, we present an observational investigation of the Pillar IV and an ionized knot HH 216 in the Eagle Nebula (M16). Pillar IV is known to host a C…

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