Multi-zone non-thermal radiative model for stellar bowshocks

Author： del Palacio S.   Bosch-Ramon V.   Müller A. L.   Romero G. E.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|617|issue|A13-A13

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.617, Iss.issue, 2018-09, pp. : A13-A13

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Abstract

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.

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