The Emission from Photoionized Stellar Wind Bow Shocks

Details The Emission from Photoionized Stellar Wind Bow Shocks The Emission from Photoionized Stellar Wind Bow Shocks

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005rmxaa..41..101c&link_type=abstract

Revista Mexicana de Astronomía y Astrofísica Vol. 41, pp. 101-108 (2005) (http://www.astroscu.unam.mx/~rmaa/)

Astronomy and Astrophysics

Astrophysics

3

Ism: Herbig-Haro Objects, Ism: Jets And Outflows, Ism: Kinematics And Dynamics

Scientific paper

Photoionized stellar wind bow shocks are found in a number of different astrophysical objects compact H II regions, H II regions around runaway O stars and bow shocks around young, low mass stars within photoionized regions. We present a formulation for calculating the emission measure from analytic, thin shell stellar wind bow shock models, with which simple predictions of the recombination line or the free-free emission can be made. We illustrate the predictions that can be made by calculating the emission maps that result from a model of a non-axisymmetric stellar wind bow shock.

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