Multi-zone non-thermal radiative model for stellar bowshocks

Context. Runaway stars produce bowshocks that are usually observed at infrared (IR) wavelengths. Non-thermal radio emission has been detected so far only from the bowshock of BD+43°3654, whereas the detection of non-thermal radiation from these bowshocks at high energies remains elusive. Aims. We ai...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2018-09, Vol.617, p.A13
Hauptverfasser:	del Palacio, S., Bosch-Ramon, V., Müller, A. L., Romero, G. E.
Format:	Artikel
Sprache:	eng
Schlagworte:	acceleration of particles Broadband Constraint modelling Energy Magnetic fields Morphology Multizone models outflows radiation mechanisms: non-thermal Radio emission Relativistic particles stars: massive stars: winds Stellar winds Thermal radiation Wavelengths X ray spectra
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