Add to ORKGThe very massive runaway star BD+43° 3654 (O4 If) seems to be related with a bow shock detected by the MSX mission, that would be the result of the interaction of the strong stellar wind with the ambient matter. Shock-accelerated electrons will cool through synchrotron radiation producing a non-thermal radio source, yet never detected in such scenario. While new Very Large Array observations are carried out, we have examined archive data and present here the findings.Fil: Peri, Cintia Soledad. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Benaglia, Paula. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro ...
Aims. This work aims at investigating the interaction of HD 192281 (O5 Vn((f))p) with its local ISM....
Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic vel...
Context. Runaway stars produce bowshocks that are usually observed at infrared (IR) wavelengths. Non...
The very massive runaway star BD+43° 3654 (O4 If) seems to be related with a bow shock detected by t...
Context. The environs of massive, early-type stars have been inspected in recent years in the search...
The bow shock produced by the high-mass runaway star BD +43° 3654 (Comerón & Pasquali 2007) has been...
We present a study of the radio emission from a massive runaway star. The star forms a bow shock tha...
Context. The environs of massive, early-type stars have been inspected in recent years in the search...
Non-thermal radiation has been predicted within bow shocks around runaway stars by recent theoretica...
Context. In recent years, winds from massive stars have been considered promising sites for investig...
Runaway, massive stars are not among the most numerous. However, the bow shocks built by their super...
We present a deep radio-polarimetric observation of the stellar bow shock EB27 associated with the m...
The latest survey of stellar bow shocks (Peri et al. 2012, A&A, 538, 108) lists 28 candidates detect...
Recent observations toward the O2 If* star HD 93129A have revealed important non-thermal radio emiss...
Aims.We investigate the star BD+43° 3654 and the possibility that it may have originated in the mass...
Aims. This work aims at investigating the interaction of HD 192281 (O5 Vn((f))p) with its local ISM....
Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic vel...
Context. Runaway stars produce bowshocks that are usually observed at infrared (IR) wavelengths. Non...
The very massive runaway star BD+43° 3654 (O4 If) seems to be related with a bow shock detected by t...
Context. The environs of massive, early-type stars have been inspected in recent years in the search...
The bow shock produced by the high-mass runaway star BD +43° 3654 (Comerón & Pasquali 2007) has been...
We present a study of the radio emission from a massive runaway star. The star forms a bow shock tha...
Context. The environs of massive, early-type stars have been inspected in recent years in the search...
Non-thermal radiation has been predicted within bow shocks around runaway stars by recent theoretica...
Context. In recent years, winds from massive stars have been considered promising sites for investig...
Runaway, massive stars are not among the most numerous. However, the bow shocks built by their super...
We present a deep radio-polarimetric observation of the stellar bow shock EB27 associated with the m...
The latest survey of stellar bow shocks (Peri et al. 2012, A&A, 538, 108) lists 28 candidates detect...
Recent observations toward the O2 If* star HD 93129A have revealed important non-thermal radio emiss...
Aims.We investigate the star BD+43° 3654 and the possibility that it may have originated in the mass...
Aims. This work aims at investigating the interaction of HD 192281 (O5 Vn((f))p) with its local ISM....
Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic vel...
Context. Runaway stars produce bowshocks that are usually observed at infrared (IR) wavelengths. Non...