IAR 05382
INSTITUTO ARGENTINO DE RADIOASTRONOMIA
Unidad Ejecutora - UE
artículos
Título:
Analysis of the spectral energy distribution from a runaway star bow shock
Autor/es:
PERI, C.S.; A. T. ARAUDO; BENAGLIA, P.; ROMERO, GUSTAVO E.; J. MARTÍ
Revista:
REVISTA MEXICANA DE ASTRONOMÃA Y ASTROFÃSICA
Editorial:
UNIV NACIONAL AUTONOMA MEXICO
Referencias:
Lugar: Mexico; Año: 2011 vol. 40 p. 156 - 156
ISSN:
0185-1101
Resumen:
The bow shock produced by the high-mass runaway star BD +43° 3654 (Comerón & Pasquali 2007) has been detected as a non-thermal radio source (S_ν ∝ ν^{-α}, =0.5) and it is the first one of that type ever observed (Benaglia et al. 2010). The non-thermal detection provides evidence of the presence of a magnetic field and relativistic electrons. This population of relativistic particles can produce high-energy (HE) emission.
