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Thomas M. Tauris

Identifiers

  • name variant Thomas M. Tauris 0.60 · backfill

Papers (27)

  1. Improved proper motion and gravity tests with PSR J1913+1102 astro-ph.HE · 2026 · author #5
  2. Deep Adaptive Optics Imaging Rules Out a Helium Star Companion to PSR J1928+1815 astro-ph.SR · 2026 · author #5
  3. The Science of the Einstein Telescope gr-qc · 2025 · author #288
  4. Observatory science with eXTP astro-ph.HE · 2018 · author #20
  5. Accretion in Strong Field Gravity with eXTP astro-ph.HE · 2018 · author #93
  6. Black holes, gravitational waves and fundamental physics: a roadmap gr-qc · 2018 · author #47
  7. Progenitors of gravitational wave mergers: Binary evolution with the stellar grid-based code ComBinE astro-ph.SR · 2018 · author #2
  8. Reconciling optical and radio observations of the binary millisecond pulsar PSR J1640+2224 astro-ph.SR · 2017 · author #6
  9. A Massive-born Neutron Star with a Massive White Dwarf Companion astro-ph.HE · 2017 · author #5
  10. Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity astro-ph.HE · 2017 · author #4
  11. Novel modelling of ultra-compact X-ray binary evolution - stable mass transfer from white dwarfs to neutron stars astro-ph.SR · 2017 · author #2
  12. Light-curve and spectral properties of ultra-stripped core-collapse supernovae leading to binary neutron stars astro-ph.HE · 2016 · author #6
  13. Recycled Pulsars: Spins, Masses and Ages astro-ph.SR · 2016 · author #1
  14. Models of low-mass helium white dwarfs including gravitational settling, thermal and chemical diffusion, and rotational mixing astro-ph.SR · 2016 · author #3
  15. The millisecond pulsar mass distribution: Evidence for bimodality and constraints on the maximum neutron star mass astro-ph.HE · 2016 · author #2
  16. Constraining the ellipticity of strongly magnetized neutron stars powering superluminous supernovae astro-ph.HE · 2016 · author #2
  17. Ultra-stripped supernovae: progenitors and fate astro-ph.SR · 2015 · author #1
  18. Understanding the Neutron Star Population with the SKA astro-ph.HE · 2014 · author #1
  19. Direct formation of millisecond pulsars from rotationally delayed accretion-induced collapse of massive white dwarfs astro-ph.SR · 2013 · author #2
  20. Evolution towards and beyond accretion-induced collapse of massive white dwarfs and formation of millisecond pulsars astro-ph.SR · 2013 · author #1
  21. Formation of black widows and redbacks -- two distinct populations of eclipsing binary millisecond pulsars astro-ph.SR · 2013 · author #3
  22. A Massive Pulsar in a Compact Relativistic Binary astro-ph.HE · 2013 · author #4
  23. Formation of millisecond pulsars with CO white dwarf companions - II. Accretion, spin-up, true ages and comparison to MSPs with He white dwarf companions astro-ph.SR · 2012 · author #1
  24. Five and a half roads to form a millisecond pulsar astro-ph.HE · 2011 · author #1
  25. Formation of millisecond pulsars with CO white dwarf companions - I. PSR J1614-2230: Evidence for a neutron star born massive astro-ph.SR · 2011 · author #1
  26. Torque Decay in the Pulsar (P,P_dot) Diagram. Effects of Crustal Ohmic Dissipation and Alignment astro-ph · 2001 · author #1
  27. On the Binding Energy Parameter of Common Envelope Evolution. Dependency on the Definition of the Stellar Core Boundary during Spiral-in astro-ph · 2001 · author #1

Mentions

  • 2606.19276 #5 · arxiv_oai · confidence 0.70 Thomas M. Tauris
  • 2604.03385 #5 · arxiv_oai · confidence 0.70 Thomas M. Tauris
  • 1505.00270 #1 · backfill · confidence 0.70 Thomas M. Tauris
  • 1501.00005 #1 · backfill · confidence 0.70 Thomas M. Tauris
  • 1311.3478 #2 · backfill · confidence 0.70 Thomas M. Tauris
  • 1308.4887 #1 · backfill · confidence 0.70 Thomas M. Tauris
  • 1308.4107 #3 · backfill · confidence 0.70 Thomas M. Tauris
  • 1304.6875 #4 · backfill · confidence 0.70 Thomas M. Tauris
  • 1206.1862 #1 · backfill · confidence 0.70 Thomas M. Tauris
  • 1106.0897 #1 · backfill · confidence 0.70 Thomas M. Tauris
  • 1103.4996 #1 · backfill · confidence 0.70 Thomas M. Tauris

Frequent Coauthors