Interstellar gas and X-rays toward the Young supernova remnant RCW 86; pursuit of the origin of the thermal and non-thermal X-ray

We have analyzed the atomic and molecular gas using the 21 cm HI and 2.6/1.3 mm CO emissions toward the young supernova remnant (SNR) RCW 86 in order to identify the interstellar medium with which the shock waves of the SNR interact. We have found an HI intensity depression in the velocity range bet...

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Detalles Bibliográficos
Autores principales: Sano, H., Reynoso, E.M., Mitsuishi, I., Nakamura, K., Furukawa, N., Mruganka, K., Fukuda, T., Yoshiike, S., Nishimura, A., Ohama, A., Torii, K., Kuwahara, T., Okuda, T., Yamamoto, H., Tachihara, K., Fukui, Y.
Formato: JOUR
Materias:
Cosmic rays
ISM: clouds
ISM: individual objects (RCW 86)
ISM: supernova remnants
X-rays: ISM
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_22144048_v15_n_p1_Sano
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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