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J. M. D. Kruijssen

Identifiers

  • name variant J. M. D. Kruijssen 0.60 · backfill

Papers (22)

  1. Young massive star cluster formation in the Galactic Centre is driven by global gravitational collapse of high-mass molecular clouds astro-ph.GA · 2019 · author #18
  2. Optical IFU spectroscopy of a bipolar microquasar jet in NGC 300 astro-ph.HE · 2019 · author #11
  3. Dense gas is not enough: environmental variations in the star formation efficiency of dense molecular gas at 100pc scales in M51 astro-ph.GA · 2019 · author #17
  4. 'The Brick' is not a brick: A comprehensive study of the structure and dynamics of the Central Molecular Zone cloud G0.253+0.016 astro-ph.GA · 2019 · author #5
  5. Feedback from massive stars at low metallicities: MUSE observations of N44 and N180 in the Large Magellanic Cloud astro-ph.GA · 2018 · author #5
  6. A 50 pc scale view of star formation efficiency across NGC 628 astro-ph.GA · 2018 · author #3
  7. Star formation in a high-pressure environment: An SMA view of the Galactic centre dust ridge astro-ph.GA · 2017 · author #6
  8. Simultaneous low- and high-mass star formation in a massive protocluster: ALMA observations of G11.92-0.61 astro-ph.GA · 2017 · author #5
  9. A revised planetary nebula luminosity function distance to NGC 628 using MUSE astro-ph.GA · 2016 · author #5
  10. The link between solenoidal turbulence and slow star formation in G0.253+0.016 astro-ph.SR · 2016 · author #4
  11. The link between turbulence, magnetic fields, filaments, and star formation in the Central Molecular Zone cloud G0.253+0.016 astro-ph.GA · 2016 · author #4
  12. Seeding the Galactic Centre gas stream: gravitational instabilities set the initial conditions for the formation of protocluster clouds astro-ph.GA · 2016 · author #3
  13. Comparing Young Massive Clusters and their Progenitor Clouds in the Milky Way astro-ph.GA · 2016 · author #4
  14. Molecular gas kinematics within the central 250 pc of the Milky Way astro-ph.GA · 2016 · author #3
  15. Is the Escape Velocity in Star Clusters Linked to Extended Star Formation Histories? Using NGC 7252: W3 as a Test Case astro-ph.GA · 2016 · author #6
  16. Tracing the Conversion of Gas into Stars in Young Massive Cluster Progenitors astro-ph.GA · 2015 · author #4
  17. A cluster in the making: ALMA reveals the initial conditions for high-mass cluster formation astro-ph.GA · 2015 · author #4
  18. Absorption Filaments Towards the Massive Clump G0.253+0.016 astro-ph.GA · 2014 · author #12
  19. Turbulence sets the initial conditions for star formation in high-pressure environments astro-ph.GA · 2014 · author #4
  20. G0.253+0.016: A centrally condensed, high-mass protocluster astro-ph.GA · 2014 · author #11
  21. Candidate super star cluster progenitor gas clouds possibly triggered by close passage to Sgr A* astro-ph.GA · 2013 · author #2
  22. Can habitable planets form in clustered environments? astro-ph.SR · 2012 · author #2

Mentions

  • 1409.3640 #12 · backfill · confidence 0.70 J. M. D. Kruijssen
  • 1409.0935 #4 · backfill · confidence 0.70 J. M. D. Kruijssen
  • 1403.0996 #11 · backfill · confidence 0.70 J. M. D. Kruijssen
  • 1304.2397 #2 · backfill · confidence 0.70 J. M. D. Kruijssen
  • 1209.2136 #2 · backfill · confidence 0.70 J. M. D. Kruijssen

Frequent Coauthors