Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Greco, E."'
Publikováno v:
ApJ 951 103 (2023)
Young supernova remnants (SNRs) shocks are believed to be the main sites of galactic cosmic rays production, showing X-ray synchrotron dominated spectra in the vicinity of their shock. While a faint thermal signature left by the shocked interstellar
Externí odkaz:
http://arxiv.org/abs/2302.02346
Autor:
Cosentino, G., Jiménez-Serra, I., Tan, J. C., Henshaw, J. D., Barnes, A. T., Law, C. -Y., Zeng, S., Fontani, F., Caselli, P., Viti, S., Zahorecz, S., Rico-Villas, F., Megías, A., Miceli, M., Orlando, S., Ustamujic, S., Greco, E., Peres, G., Bocchino, F., Fedriani, R., Gorai, P., Testi, L., Martín-Pintado, J.
Supernova remnants (SNRs) contribute to regulate the star formation efficiency and evolution of galaxies. As they expand into the interstellar medium (ISM), they transfer vast amounts of energy and momentum that displace, compress and heat the surrou
Externí odkaz:
http://arxiv.org/abs/2201.03008
Autor:
Orlando, S., Miceli, M., Ustamujic, S., Tutone, A., Greco, E., Petruk, O., Bocchino, F., Peres, G.
According to the most popular model for the origin of cosmic rays (CRs), supernova remnants (SNRs) are the site where CRs are accelerated. Observations across the electromagnetic spectrum support this picture through the detection of non-thermal emis
Externí odkaz:
http://arxiv.org/abs/2012.13394
Publikováno v:
A&A 649, A14 (2021)
The morphology and the distribution of material observed in SNRs reflect the interaction of the SN blast wave with the ambient environment, the physical processes associated with the SN explosion and the internal structure of the progenitor star. IC
Externí odkaz:
http://arxiv.org/abs/2012.08017