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M. Kohandel

3 papers here

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

author position
  • middle author3

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

fields
  • astro-ph.GA3
ORCID 0000-0003-1041-7865
same name
  • M. Kohandel — 11 papers, h 29
  • M. Kohandel — 1 paper, h 11

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

most citedALMA hints at the presence of turbulent disk galaxies at z > 5

45 citations · 78 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2024★ 32 cited

The ALMA-ALPAKA survey II. Evolution of turbulence in galaxy disks across cosmic time: difference between cold and warm gas

F. Rizzo, C. Bacchini, M. Kohandel +8

The gas in the interstellar medium (ISM) of galaxies is supersonically turbulent. Measurements of turbulence typically rely on cold gas emission lines for low-z galaxies and warm i…

astro-ph.GA2023★ 1 cited

Spatially resolved Kennicutt-Schmidt relation at z~7 and its connection with the interstellar medium properties

Livia Vallini, Joris Witstok, Laura Sommovigo +7

We exploit moderately resolved [OIII], [CII] and dust continuum ALMA observations to derive the gas density (n), the gas-phase metallicity (Z) and the deviation from the Kennic…

astro-ph.GA2023★ 45 cited

ALMA hints at the presence of turbulent disk galaxies at z > 5

E. Parlanti, S. Carniani, A. Pallottini +5

High-redshift galaxies are expected to be more turbulent than local galaxies because of their smaller size and higher star formation and thus stronger feedback from star formation,…

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