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researcher

R. Simon

48 papers hereh-index 324k citations160 works total

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

author position
  • first author1
  • middle author37
  • last author4

Across the 42 of 48 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA37
  • astro-ph5
  • astro-ph.SR3
  • astro-ph.CO2
  • astro-ph.IM1
same name
  • R. Simon — 46 papers, h 37
  • R. Simon — 24 papers, h 11
  • R. Simon — 13 papers, h 32
  • R. Simon — 13 papers, h 9
  • R. Simon — 11 papers, h 9
  • R. Simon — 8 papers, h 2

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
20052023
most citedInfrared Dark Clouds: precursors to star clusters

471 citations · 3.3k across the 48 of their papers we have counts for

collaborators
Showing 2012 · astro-ph.GAShow all

4 papers · 2 filters

astro-ph.GA2012★ 45 cited

Globules and pillars seen in the [CII] 158 micron line with SOFIA

N. Schneider, R. Güsten, P. Tremblin +22

Molecular globules and pillars are spectacular features, found only in the interface region between a molecular cloud and an HII-region. Impacting Far-ultraviolet (FUV) radiation c…

astro-ph.GA2012★ 29 cited

The ionized and hot gas in M17 SW: SOFIA/GREAT THz observations of [C II] and 12CO J=13-12

J. P. Perez-Beaupuits, H. Wiesemeyer, V. Ossenkopf +5

With new THz maps that cover an area of ~3.3x2.1 pc^2 we probe the spatial distribution and association of the ionized, neutral and molecular gas components in the M17 SW nebula. W…

astro-ph.GA2012

Dynamics and PDR properties in IC1396A

Yoko Okada, Rolf Güsten, Miguel Angel Requena-Torres +7

We investigate the gas dynamics and the physical properties of photodissociation regions (PDRs) in IC1396A, which is an illuminated bright-rimmed globule with internal structures c…

astro-ph.GA2012★ 16 cited

The structure of hot gas in Cepheus B

B. Mookerjea, V. Ossenkopf, O. Ricken +6

By observing radiation-affected gas in the Cepheus B molecular cloud we probe whether the sequential star formation in this source is triggered by the radiation from newly formed s…

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