Runaway, massive stars are not among the most numerous. However, the bow shocks built by their supersonic movement in the interstellar medium have been detected in the infrared range in many cases. Most recently, the stellar bow shocks have been proposed as particle acceleration sites, as radio data analysis at high angular resolution have shown. We present results of different manifestations of the stellar bowshock phenomenon, revealed from modern IR databases.Las estrellas masivas fugitivas no son de las más numerosas. Sin embargo, los bowshocks formados debido a su movimiento supersónico en el medio interestelar han sido detectados en el rango infrarrojo en muchos casos. Muy recientemente, estos bowshocks estelares fueron propuestos como...
Massive stars moving at supersonic peculiar velocities through the interstellar medium (ISM) can cre...
Context. Runaway massive stars are O-and B-type stars with high spatial velocities with respect to t...
Context. The environs of massive, early-type stars have been inspected in recent years in the search...
Context. Stellar bow shocks have been studied not only observationally, but also theoretically since...
The latest survey of stellar bow shocks (Peri et al. 2012, A&A, 538, 108) lists 28 candidates detect...
Context. Bow shocks are produced by many astrophysical objects where shock waves are present. Stella...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ...
Context. Stellar bow shocks have been studied not only observationally, but also theoretically since...
© 2012. The American Astronomical Society. All rights reserved. Printed in the U.S.A.This work was s...
We present a study of the radio emission from a massive runaway star. The star forms a bow shock tha...
Runaway stars produce shocks when passing through interstellar medium at supersonic velocities. Bow ...
Runaway masive stars are O- and B-type stars with large peculiar veloci- ties. Runaway OB stars can ...
Context. Bow shocks are produced by many astrophysical objects where shock waves are present. Stella...
International audienceMassive stars that have been ejected from their parent cluster and supersonica...
Context. Bow shocks are produced by many astrophysical objects where shock waves are present. Stella...
Massive stars moving at supersonic peculiar velocities through the interstellar medium (ISM) can cre...
Context. Runaway massive stars are O-and B-type stars with high spatial velocities with respect to t...
Context. The environs of massive, early-type stars have been inspected in recent years in the search...
Context. Stellar bow shocks have been studied not only observationally, but also theoretically since...
The latest survey of stellar bow shocks (Peri et al. 2012, A&A, 538, 108) lists 28 candidates detect...
Context. Bow shocks are produced by many astrophysical objects where shock waves are present. Stella...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ...
Context. Stellar bow shocks have been studied not only observationally, but also theoretically since...
© 2012. The American Astronomical Society. All rights reserved. Printed in the U.S.A.This work was s...
We present a study of the radio emission from a massive runaway star. The star forms a bow shock tha...
Runaway stars produce shocks when passing through interstellar medium at supersonic velocities. Bow ...
Runaway masive stars are O- and B-type stars with large peculiar veloci- ties. Runaway OB stars can ...
Context. Bow shocks are produced by many astrophysical objects where shock waves are present. Stella...
International audienceMassive stars that have been ejected from their parent cluster and supersonica...
Context. Bow shocks are produced by many astrophysical objects where shock waves are present. Stella...
Massive stars moving at supersonic peculiar velocities through the interstellar medium (ISM) can cre...
Context. Runaway massive stars are O-and B-type stars with high spatial velocities with respect to t...
Context. The environs of massive, early-type stars have been inspected in recent years in the search...