Evidence of a Mira-like tail and bow shock about the semi-regular variable V CVn from four decades of polarization measurements.
Polarization is a powerful tool for understanding stellar atmospheres and circumstellar environments. Mira and semi-regular variable stars have been observed for decades and some are known to be polarimetrically variable, however, the semi-regular variable V Canes Venatici displays an unusually large, unexplained amount of polarization. We present ten years of optical polarization observations obtained with the HPOL instrument, supplemented by published observations spanning a total interval of about forty years for V CVn. We find that V CVn shows large polarization variations ranging from 1 - 6%. We also find that for the past forty years the position angle measured for V CVn has been virtually constant suggesting a long-term, stable, asymmetric structure about the star. We suggest that this asymmetry is caused by the presence of a stellar wind bow shock and tail, consistent with the star's large space velocity.
Hilding R. Neilson, Richard Ignace, Beverly J. Smith, Gary Henson, and Alyssa M. Adams. "Evidence of a Mira-like tail and bow shock about the semi-regular variable V CVn from four decades of polarization measurements." Astronomy & Astrophysics 568 (2014): A88.
Available at: http://works.bepress.com/richard_ignace/9
Reproduced with permission from Astronomy & Astrophysics, Copyright © ESO 2014.