High-sensitivity radio study of the non-thermal stellar bow shock EB27

We present a deep radio-polarimetric observation of the stellar bow shock EB27 associated to the massive star BD+43 3654. This is the only stellar bow shock confirmed to have non-thermal radio emission. We used the Jansky Very Large Array in S band (2 - 4GHz) to test whether this synchrotron emissio...

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Veröffentlicht in:	arXiv.org 2021-03
Hauptverfasser:	Benaglia, Paula, Santiago del Palacio, Hales, Christopher, Colazo, Marcelo E
Format:	Artikel
Sprache:	eng
Schlagworte:	Charged particles Emission analysis Linear polarization Massive stars Morphology Physics - Astrophysics of Galaxies Physics - High Energy Astrophysical Phenomena Physics - Solar and Stellar Astrophysics Polarimetry Radio emission Sensitivity Synchrotrons
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