37 citations · 82 across the 7 of their papers we have counts for
7 papers
New line-driven wind mass-loss rates for OB stars with metallicities down to
Jiri Krticka, Jiri Kubat, Iva Krtickova
We provide new line-driven wind models for OB stars with metallicities down to . The models were calculated with our global wind code METUJE, which solves the hydrod…
Hot subdwarf wind models with accurate abundances II. Helium-dominated merger products CD-46 8926 and CD-51 11879
J. Krticka, I. Krtickova, J. Janik +3
We aim to understand the influence of evolutionary modified surface abundances on the strength of the stellar wind in the helium-dominated subdwarfs CD-46 8926 and CD-51 11879. We…
New mass-loss rates of Magellanic Cloud B supergiants from global wind models
J. Krticka, J. Kubat, I. Krtickova
We provide global models of line-driven winds of B supergiants for metallicities corresponding to the Large and Small Magellanic Clouds. The velocity and density structure of the m…
Stellar wind models of central stars of planetary nebulae
J. Krticka, J. Kubat, I. Krtickova
Fast line-driven stellar winds play an important role in the evolution of planetary nebulae. We provide global hot star wind models of central stars of planetary nebulae. The model…
Hot subdwarf wind models with accurate abundances I. Hydrogen dominated stars HD 49798 and BD+182647
J. Krticka, J. Janik, I. Krtickova +5
Hot subdwarfs are helium burning objects in late stages of their evolution. These stars can develop winds driven by light absorption in the lines of heavier elements. The wind stre…
Stellar wind models of subluminous hot stars
J. Krticka, J. Kubat, I. Krtickova
Mass-loss rate is one of the most important stellar parameters. We aim to provide mass-loss rates as a function of subdwarf parameters and to apply the formula for individual subdw…