The first large blue-wavelength spectroscopic census of bowshock central stars provides Teff, log g, and v sin i for 103 OB stars and argues that runaway bowshock stars favor the dynamical ejection channel.
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Fundamental Parameters for Central Stars of 103 Infrared Bowshock Nebulae
The first large blue-wavelength spectroscopic census of bowshock central stars provides Teff, log g, and v sin i for 103 OB stars and argues that runaway bowshock stars favor the dynamical ejection channel.