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M. Padovani

84 papers hereh-index 387.5k citations151 works total

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

author position
  • first author15
  • middle author35
  • last author8

Across the 58 of 84 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE36
  • astro-ph.GA30
  • astro-ph.SR17
  • astro-ph.IM1
same name
  • M. Padovani — 18 papers, h 4
  • 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
20092023
most citedCosmic-ray ionization of molecular clouds

387 citations · 4.6k across the 82 of their papers we have counts for

collaborators
Showing 2014Show all

3 papers · 1 filter

astro-ph.GA2014★ 60 cited

The Importance of the Magnetic Field from an SMA-CSO-Combined Sample of Star-Forming Regions

Patrick M. Koch, Ya-Wen Tang, Paul T. P. Ho +14

Submillimeter dust polarization measurements of a sample of 50 star-forming regions, observed with the SMA and the CSO covering pc-scale clouds to mpc-scale cores, are analyzed in…

astro-ph.GA2014★ 55 cited

The role of cosmic rays on magnetic field diffusion and the formation of protostellar discs

Marco Padovani, Daniele Galli, Patrick Hennebelle +2

The formation of protostellar discs is severely hampered by magnetic braking, as long as magnetic fields remain frozen in the gas. The latter condition depends on the levels of ion…

astro-ph.GA2014★ 209 cited

Magnetic Fields and Massive Star Formation

Qizhou Zhang, Keping Qiu, Josep M. Girart +17

Massive stars (M>8 \msun) typically form in parsec-scale molecular clumps that collapse and fragment, leading to the birth of a cluster of stellar objects. We investigate the r…

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