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E. Muller

11 papers hereh-index 11694 citations13 works total

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

author position
  • first author3
  • middle author5

Across the 8 of 11 papers where every author was matched, so the position is known.

fields
  • astro-ph5
  • astro-ph.GA4
  • astro-ph.CO1
  • astro-ph.SR1
same name
  • E. Muller — 45 papers, h 26
  • E. Muller — 12 papers, h 20
  • E. Muller — 9 papers, h 1
  • E. Muller — 6 papers, h 6
  • E. Muller — 5 papers, h 17
  • E. Muller — 3 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
20022017
most citedPhysical Properties of Giant Molecular Clouds in the Large Magellanic Cloud

126 citations · 623 across the 11 of their papers we have counts for

collaborators
Showing 2009 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2009★ 85 cited

Molecular and Atomic Gas in the Large Magellanic Cloud II. Three-dimensional Correlation between CO and HI

Y. Fukui, A. Kawamura, T. Wong +10

We compare the CO J =(1-0) and HI emission in the Large Magellanic Cloud (LMC) in three dimensions, i.e. including a velocity axis in addition to the two spatial axes, with the aim…

astro-ph.GA2009★ 38 cited

The Influence of Far-Ultraviolet Radiation on the Properties of Molecular Clouds in the 30 Dor Region of the Large Magellanic Cloud

Jorge L. Pineda, Juergen Ott, Ulrich Klein +3

We present a complete 12CO J = 1-0 map of the prominent molecular ridge in the Large Magellanic Cloud (LMC) obtained with the 22-m ATNF Mopra Telescope. The region stretches southw…

astro-ph.GA2009★ 50 cited

Molecular and Atomic Gas in the Large Magellanic Cloud - I. Conditions for CO Detection

T. Wong, A. Hughes, Y. Fukui +10

We analyze the conditions for detection of CO(1-0) emission in the Large Magellanic Cloud (LMC), using the recently completed second NANTEN CO survey. In particular, we investigate…

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