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M. Krause

90 papers hereh-index 292.6k citations117 works total

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

author position
  • sole author8
  • first author23
  • middle author42
  • last author13

Across the 86 of 90 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA29
  • astro-ph.HE25
  • astro-ph.CO16
  • astro-ph15
  • astro-ph.SR3
  • astro-ph.IM2
same name
  • M. Krause — 81 papers, h 32
  • M. Krause — 33 papers, h 25
  • M. Krause — 11 papers, h 11
  • M. Krause — 9 papers, h 25
  • M. Krause — 7 papers, h 7
  • M. Krause — 5 papers, h 7

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
20022026
most citedJet-induced star formation in gas-rich galaxies

248 citations · 3.8k across the 89 of their papers we have counts for

collaborators
Showing 2012 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2012★ 46 cited

Superbubble dynamics in globular cluster infancy I. How do globular clusters first lose their cold gas?

Martin Krause, Corinne Charbonnel, Thibaut Decressin +3

The picture of the early evolution of globular clusters has been significantly revised in recent years. Current scenarios require at least two generations of stars of which the fir…

astro-ph.GA2012★ 18 cited

Magnetohydrodynamic stability of broad line region clouds

Martin Krause, Marc Schartmann, Andreas Burkert

Hydrodynamic stability has been a longstanding issue for the cloud model of the broad line region in active galactic nuclei. We argue that the clouds may be gravitationally bound t…

astro-ph.GA2012★ 42 cited

Feedback by massive stars and the emergence of superbubbles I. Energy efficiency & Vishniac instabilities

Martin Krause, Katharina Fierlinger, Roland Diehl +3

We study the evolution of isolated and merging interstellar bubbles of three stars (25, 32 and 60 M\odot) in a homogeneous background medium with a density of 10 mp /ccm via 3D-hyd…

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