pith. sign in

Jon O. Sundqvist

Identifiers

  • name variant Jon O. Sundqvist 0.60 · backfill

Papers (15)

  1. Multi-dimensional, time-dependent approximate NLTE unified model atmospheres with winds for hot, massive stars astro-ph.SR · 2026 · author #2
  2. Characterizing the turbulent porosity of stellar-wind structure generated by the line-deshadowing instability astro-ph.SR · 2017 · author #2
  3. An `Analytic Dynamical Magnetosphere' formalism for X-ray and optical emission from slowly rotating magnetic massive stars astro-ph.SR · 2016 · author #3
  4. Effect of scattering on the transonic solution topology and intrinsic variability of line-driven stellar winds astro-ph.SR · 2015 · author #1
  5. Measuring the shock-heating rate in the winds of O stars using X-ray line spectra astro-ph.SR · 2014 · author #5
  6. Constraining general massive-star physics by exploring the unique properties of magnetic O-stars: Rotation, macroturbulence, and sub-surface convection astro-ph.SR · 2014 · author #1
  7. Constraints on porosity and mass loss in O-star winds from modeling of X-ray emission line profile shapes astro-ph.SR · 2013 · author #3
  8. Thin-shell mixing in radiative wind-shocks and the Lx-Lbol scaling of O-star X-rays astro-ph.SR · 2012 · author #2
  9. First 3D MHD simulation of a massive-star magnetosphere with application to H\alpha emission from \theta^1 Ori C astro-ph.SR · 2012 · author #2
  10. Clumping in the inner winds of hot, massive stars from hydrodynamical line-driven instability simulations astro-ph.SR · 2012 · author #1
  11. A dynamical magnetosphere model for periodic Halpha emission from the slowly rotating magnetic O star HD191612 astro-ph.SR · 2012 · author #1
  12. A generalised porosity formalism for isotropic and anisotropic effective opacity and its effects on X-ray line attenuation in clumped O star winds astro-ph.SR · 2011 · author #1
  13. The nature and consequences of clumping in hot, massive star winds astro-ph.SR · 2011 · author #1
  14. A proper description of clumping in hot star winds: the key to obtaining reliable mass-loss rates? astro-ph.SR · 2010 · author #1
  15. OB-stars as extreme condition test beds astro-ph.SR · 2010 · author #2

Mentions

  • 1409.0856 #5 · backfill · confidence 0.70 Jon O. Sundqvist
  • 1409.0028 #1 · backfill · confidence 0.70 Jon O. Sundqvist
  • 1305.5595 #3 · backfill · confidence 0.70 Jon O. Sundqvist
  • 1212.4235 #2 · backfill · confidence 0.70 Jon O. Sundqvist
  • 1210.5298 #2 · backfill · confidence 0.70 Jon O. Sundqvist
  • 1210.1861 #1 · backfill · confidence 0.70 Jon O. Sundqvist
  • 1203.1050 #1 · backfill · confidence 0.70 Jon O. Sundqvist
  • 1111.1762 #1 · backfill · confidence 0.70 Jon O. Sundqvist
  • 1110.0485 #1 · backfill · confidence 0.70 Jon O. Sundqvist
  • 1010.3987 #1 · backfill · confidence 0.70 Jon O. Sundqvist
  • 1009.0364 #2 · backfill · confidence 0.70 Jon O. Sundqvist

Frequent Coauthors