X-ray study of bow shocks in runaway stars

Autor: Paula Benaglia, Michaël De Becker, Gustavo E. Romero, C. S. Peri, M. V. del Valle

Publikováno v: SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET

Massive runaway stars produce bow shocks through the interaction of their winds with the interstellar medium, with the prospect for particle acceleration by the shocks. These objects are consequently candidates for non-thermal emission. Our aim is to

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6c83abe9fd1863483e38e554acb82ab5
https://doi.org/10.1093/mnras/stx1826

E-BOSS: An Extensive stellar BOw Shock Survey. II. Catalogue second release

Autor: N. L. Isequilla, Paula Benaglia, C. S. Peri

Publikováno v: SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP

Context. Stellar bow shocks have been studied not only observationally, but also theoretically since the late 1980s. Only a few catalogues of them exist. The bow shocks show emission along all the electromagnetic spectrum, but they are detected more

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a5693bcd8e5615be8d993133a0a90273

E-BOSS: an Extensive stellar BOw Shock Survey. I: Methods and First Catalogue

Autor: D. P. Brookes, N. L. Isequilla, Ian R. Stevens, C. S. Peri, Paula Benaglia

Context. Bow shocks are produced by many astrophysical objects where shock waves are present. Stellar bow shocks, generated by runaway stars, have been previously detected in small numbers and well-studied. Along with progress in model development an

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5a1bf4e1f917aefb244d33cf7ed0cee7
http://arxiv.org/abs/1109.3689

EVIDENCE OF NON-THERMAL X-RAY EMISSION FROM HH 80

Autor: Paula Benaglia, Marco Miceli, C. S. Peri, J. F. Albacete-Colombo, Javier López-Santiago, Rosaria Bonito, E. de Castro

Publikováno v: E-Prints Complutense. Archivo Institucional de la UCM
instname
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid

Protostellar jets appear at all stages of star formation when the accretion process is still at work. Jets travel at velocities of hundreds of km s -1, creating strong shocks when interacting with the interstellar medium. Several cases of jets have b

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::78b5fbdbd78e50966d28381fd78560bd
https://doi.org/10.1088/2041-8205/776/2/l22