pith. sign in

N. Mennekens

Identifiers

  • name variant N. Mennekens 0.60 · backfill

Papers (24)

  1. The spin rates and spin evolution of the O components in WR+O binaries astro-ph.SR · 2017 · author #2
  2. Observational signatures of past mass-exchange episodes in massive binaries: The case of LSS 3074 astro-ph.SR · 2017 · author #6
  3. A comparison between observed Algol-type double stars in the Solar neighborhood and evolutionary computations of galactic case A binaries with a B-type primary at birth astro-ph.SR · 2016 · author #1
  4. Evolution of intermediate mass and massive binary stars: physics, mass loss, and rotation astro-ph.SR · 2016 · author #2
  5. The delayed time distribution of massive double compact star mergers astro-ph.SR · 2016 · author #1
  6. Massive star population synthesis with binaries astro-ph.SR · 2015 · author #2
  7. PopCORN: Hunting down the differences between binary population synthesis codes astro-ph.SR · 2013 · author #3
  8. Massive double compact object mergers: gravitational wave sources and r-process-element production sites astro-ph.SR · 2013 · author #1
  9. No unique quadratic ephemeris for VW Cep astro-ph.SR · 2013 · author #3
  10. Progenitors of Supernovae Type Ia astro-ph.HE · 2013 · author #6
  11. The effect of intermediate mass close binaries on the chemical evolution of Globular Clusters II astro-ph.GA · 2013 · author #1
  12. Blue supergiant progenitor models of Type II supernovae astro-ph.SR · 2012 · author #2
  13. Progenitors of type Ia supernovae and the metallicity distribution of G-type dwarfs astro-ph.SR · 2012 · author #1
  14. POPCORN: A comparison of binary population synthesis codes astro-ph.SR · 2012 · author #3
  15. Two distributions shedding light on supernova Ia progenitors: delay times and G-dwarf metallicities astro-ph.SR · 2012 · author #1
  16. The effect of intermediate mass close binaries on the chemical evolution of Globular Clusters astro-ph.GA · 2011 · author #2
  17. Delay time distribution of type Ia supernovae: theory vs. observation astro-ph.SR · 2010 · author #1
  18. Mass loss out of close binaries. II astro-ph.SR · 2010 · author #3
  19. The delay time distribution of type Ia supernovae: a comparison between theory and observation astro-ph.SR · 2010 · author #1
  20. Mass loss out of close binaries astro-ph.SR · 2009 · author #3
  21. Spin-up and hot spots can drive mass out of a binary astro-ph · 2008 · author #4
  22. On the origin and evolutionary state of RZ Cas, KO Aql and S Equ astro-ph · 2008 · author #1
  23. Binary populations and stellar dynamics in young clusters astro-ph · 2008 · author #4
  24. Stellar dynamics in young clusters: the formation of massive runaways and very massive runaway mergers astro-ph · 2007 · author #4

Mentions

  • 1311.6503 #3 · backfill · confidence 0.70 N. Mennekens
  • 1307.0959 #1 · backfill · confidence 0.70 N. Mennekens
  • 1306.2180 #3 · backfill · confidence 0.70 N. Mennekens
  • 1302.0495 #6 · backfill · confidence 0.70 N. Mennekens
  • 1301.2423 #1 · backfill · confidence 0.70 N. Mennekens
  • 1212.4285 #2 · backfill · confidence 0.70 N. Mennekens
  • 1212.0313 #1 · backfill · confidence 0.70 N. Mennekens
  • 1211.0809 #3 · backfill · confidence 0.70 N. Mennekens
  • 1204.4358 #1 · backfill · confidence 0.70 N. Mennekens
  • 1109.2713 #2 · backfill · confidence 0.70 N. Mennekens
  • 1009.5175 #1 · backfill · confidence 0.70 N. Mennekens
  • 1008.2620 #3 · backfill · confidence 0.70 N. Mennekens
  • 1003.2491 #1 · backfill · confidence 0.70 N. Mennekens
  • 0908.2021 #3 · backfill · confidence 0.70 N. Mennekens
  • 0804.1215 #4 · backfill · confidence 0.70 N. Mennekens
  • 0802.0944 #1 · backfill · confidence 0.70 N. Mennekens
  • 0801.2674 #4 · backfill · confidence 0.70 N. Mennekens
  • 0712.3343 #4 · backfill · confidence 0.70 N. Mennekens

Frequent Coauthors