TY  - JOUR
AU  - Pereira, V.
AU  - López Santiago, J.
AU  - Miceli, M.
AU  - Bonito, R.
AU  - Castro Rubio, Elisa de
PY  - 2016
DO  - 10.1051/0004-6361/201527985
SN  - 1432-0746
UR  - https://hdl.handle.net/20.500.14352/24521
T2  - Astronomy & Astrophysics
AB  - Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic velocities and characterized by strong stellar winds may produce bow shocks that can serve as particle acceleration sites. Previous theoretical models...
LA  - eng
PB  - EDP Sciencies
KW  - Massive runaway star
KW  - O-type stars
KW  - Zeta ophiuchi
KW  - 1St detection
KW  - Origin
KW  - Rates
KW  - Field
TI  - Modeling nonthermal emission from stellar bow shocks (Research Note)
TY  - journal article
VL  - 588
ER  -