tp4.rub.de

astrospheres.tp4.rub.de

Astrospheres

http://astrospheres.tp4.rub.de//shock.php

Cosmic ray modified shocks. Renewcommand{ div}{ vec{ nabla} cdot} newcommand{ del}{ dfrac{ partial}{ partial t} } ). 169; 2014 - 2015 TP IV. Code and Design: Klaus Scherer.

astrospheres.tp4.rub.de

Astrospheres

http://astrospheres.tp4.rub.de//c-shock.php

Cosmic ray modified shocks. Renewcommand{ div}{ vec{ nabla} cdot} newcommand{ del}{ dfrac{ partial}{ partial t} } ). Cosmic ray modified shocks. 169; 2014 - 2015 TP IV. Code and Design: Klaus Scherer.

astrospheres.tp4.rub.de

Astrospheres

http://astrospheres.tp4.rub.de//conferences.php

Cosmic ray modified shocks. Renewcommand{ div}{ vec{ nabla} cdot} newcommand{ del}{ dfrac{ partial}{ partial t} } ). 169; 2014 - 2015 TP IV. Code and Design: Klaus Scherer.

astrospheres.tp4.rub.de

Astrospheres

http://astrospheres.tp4.rub.de//cosmic-ray.php

Cosmic ray modified shocks. Renewcommand{ div}{ vec{ nabla} cdot} newcommand{ del}{ dfrac{ partial}{ partial t} } ). 169; 2014 - 2015 TP IV. Code and Design: Klaus Scherer.

astrospheres.tp4.rub.de

Astrospheres

http://astrospheres.tp4.rub.de//recent.php

Cosmic ray modified shocks. Renewcommand{ div}{ vec{ nabla} cdot} newcommand{ del}{ dfrac{ partial}{ partial t} } ). Joint splinter meeting "Astrospheres around massive stars". With the Arbeitsgemeinschaft extraterrestrische Forschung. On 2015 Annual Meeting of the Astronomische Gesellschaft. At the Christian-Albrechts-Universität zu Kiel (CAU). From 14 to 18 September 2015. Organisers: D. Bomans, K. Scherer. Please send abstracts via email in the to Dominik Bomans (bomans at astro.rub.de) or Kla...

astrospheres.tp4.rub.de

Astrospheres

http://astrospheres.tp4.rub.de/imprint.php

Cosmic ray modified shocks. Renewcommand{ div}{ vec{ nabla} cdot} newcommand{ del}{ dfrac{ partial}{ partial t} } ). Institut für Theoretische Physik IV. Phone: 49 (0)234 32-26710. Fax: 49 (0)234 32-14177. Email: office@tp4.rub.de. Responsible for the content. Institut für Theoretische Physik IV. Phone: 49 (0)234 32-23458. E-Mail: kls@tp4.rub.de. 169; 2014 - 2015 TP IV. Code and Design: Klaus Scherer.

astrospheres.tp4.rub.de

Astrospheres

http://astrospheres.tp4.rub.de//old.php

Cosmic ray modified shocks. Renewcommand{ div}{ vec{ nabla} cdot} newcommand{ del}{ dfrac{ partial}{ partial t} } ). Wind Bubbles, Astrospheres and the Heliosphere: Environments and Cosmic Rays", 4 - 8 November 2013, Ruhr-Universität Bochum, Bochum, Germany. 169; 2014 - 2015 TP IV. Code and Design: Klaus Scherer.

astrospheres.tp4.rub.de

Astrospheres

http://astrospheres.tp4.rub.de/overview.php

Cosmic ray modified shocks. Renewcommand{ div}{ vec{ nabla} cdot} newcommand{ del}{ dfrac{ partial}{ partial t} } ). Winds around runaway stars, or in general, stars with a nonzero relative speed with respect to the surrounding interstellar medium (ISM), develop bullet-shaped astrospheres. The hydrodynamic large-scale structure is sketched in Fig. 1 and in more detail in Figre 2 the notation of which is described below. Taken from Scherer et al 2015a. And Scherer et al 2015b. 169; 2014 - 2015 TP IV.

astrospheres.tp4.rub.de

Astrospheres

http://astrospheres.tp4.rub.de//index.php

Cosmic ray modified shocks. Renewcommand{ div}{ vec{ nabla} cdot} newcommand{ del}{ dfrac{ partial}{ partial t} } ) Next meetings:. The Many Facets of Astrophysics - Photons, Particles, and Spacetime Annual Meeting of the German Astronomical Society,. 12 - 16. September 2016, Ruhr-Universität Bochum, Germany. Jointly Organized with the Nederlandse Astronomenclub. Jahrestagung der Astronomischen Gesellschaft, 12. - 16. September 2016, Ruhr-Universität Bochum, Deutschland. 169; 2014 - 2015 TP IV.

astrospheres.tp4.rub.de

Astrospheres

http://astrospheres.tp4.rub.de//stroemgren_radius.php

Cosmic ray modified shocks. Renewcommand{ div}{ vec{ nabla} cdot} newcommand{ del}{ dfrac{ partial}{ partial t} } ). The photons from a star with energies higher than the ionization energy (13.6 eV) of an hydrogen atom can ionize the latter. The ionization will be balanced by the recombination between protons (H. Begin{eqnarray} R S = left( frac{3}{4 pi} frac{Q star}{n {2} {H} beta {2}(T)} right) {(1/3)} end{eqnarray}. The Strömgren radius. K] Temperature of the star according to its spectral typ. The pr...