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M. Köhler

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

fields
  • astro-ph.GA3
ORCID 0000-0003-3042-1749
same name
  • M. Köhler — 2 papers, h 11
  • M. Köhler — 1 paper, h 14
  • M. Köhler — 1 paper
  • M. Köhler — 1 paper, h 9
  • M. Köhler — 1 paper, h 59
  • M. Köhler — 1 paper, h 6

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 citedThe evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point

446 citations · 482 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2015★ 10 cited

The Spatial Variation of the Cooling Lines in the Reflection Nebula NGC7023

J. Bernard-Salas, E. Habart, M. Köhler +7

Context: The north-west photo-dissociation region (PDR) in the reflection nebula NGC 7023 displays a complex structure. Filament-like condensations at the edge of the cloud can be…

astro-ph.GA2014★ 446 cited

The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point

A. P. Jones, L. Fanciullo, M. Koehler +4

Context. The evolution of amorphous hydrocarbon materials, a-C(:H), principally resulting from ultraviolet (UV) photon absorption- induced processing, are likely at the heart of th…

astro-ph.GA2014★ 26 cited

Physical structure of the photodissociation regions in NGC 7023. Observations of gas and dust emission with Herschel

M. Köhler, E. Habart, H. Arab +16

The determination of the physical conditions in molecular clouds is a key step towards our understanding of their formation and evolution of associated star formation. We investiga…

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