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Cited article:

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New γ-Ray Sources Identified in All-sky Surveys Based on Fermipy’s Advanced Algorithm

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

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Wind nebulae and supernova remnants of very massive stars

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Investigating Particle Acceleration in the Wolf–Rayet Bubble G2.4+1.4

Prachi Prajapati, Anandmayee Tej, Santiago del Palacio, Paula Benaglia, Ishwara-Chandra CH, Sarita Vig, Samir Mandal and Swarna Kanti Ghosh
The Astrophysical Journal Letters 884 (2) L49 (2019)
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Possible Association of Two Stellar Bowshocks with Unidentified Fermi Sources

E. Sánchez-Ayaso, María V. del Valle, J. Martí, G. E. Romero and P. L. Luque-Escamilla
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Systematic search for very-high-energy gamma-ray emission from bow shocks of runaway stars

H. Abdalla, A. Abramowski, F. Aharonian, et al.
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On the Absence of Non-thermal X-Ray Emission around Runaway O Stars

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The Astrophysical Journal Letters 838 (2) L19 (2017)
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X-RAY OBSERVATIONS OF BOW SHOCKS AROUND RUNAWAY O STARS. THE CASE OF ζ OPH AND BD+43°3654

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Runaway stars as cosmic ray injectors inside molecular clouds

M. V. del Valle, G. E. Romero and R. Santos-Lima
Monthly Notices of the Royal Astronomical Society 448 (1) 207 (2015)
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Systematic search for high-energy gamma-ray emission from bow shocks of runaway stars

A. Schulz, M. Ackermann, R. Buehler, M. Mayer and S. Klepser
Astronomy & Astrophysics 565 A95 (2014)
https://doi.org/10.1051/0004-6361/201423468