Energetics of nearby stellar bow shocks

P. BENAGLIA

Mar del Plata

Congreso; Reunion Anual de la Asociacion Argentina de Astronomia; 2012

Asociacion Argentina de Astronomia

(Con referato) The latest survey of stellar bow shocks (Peri et al. 2012, A&A, 538, 108) lists 28 candidates detected at IR wavelengths, associated with massive, early-type stars up to 3 kpc, along with the geometrical parameters of the structures found. I present here some considerations on the energetics involved, after the estimation of stellar wind power, infrared flux, stellar bolometric luminosity and radio flux limits for each source. The best candidates for relativistic particle acceleration are highlighted.