Multi-zone non-thermal radiative model for stellar bowshocks

<i>Context</i>. Runaway stars produce bowshocks that are usually observed at infrared (IR) wavelengths. Non-thermal radio emission has been detected so far only from the bowshock of BD+43°3654, whereas the detection of non-thermal radiation from these bowshocks at high energies remains e...

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Detalles Bibliográficos
Autores principales:	Palacio, Santiago del, Bosch Ramon, Valentí, Müller, Ana Laura, Romero, Gustavo Esteban
Formato:	Articulo Preprint
Lenguaje:	Inglés
Publicado:	2018
Materias:	Astronomía Física Ciencias Exactas Acceleration of particles Radiation mechanisms: non-thermal Stars: massive Stars: winds, outflows
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/97308 https://ri.conicet.gov.ar/11336/82398 https://www.aanda.org/articles/aa/abs/2018/09/aa33321-18/aa33321-18.html
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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