New BeppoSAX observations of the nearby prototypical starburst galaxies NGC 253 and M82 are presented. A companion paper (Cappi et al. 1998) shows that the hard (2-19 keV) spectrum of both galaxies, extracted from the source central regions, is best described by a thermal emission model with kT similar to 6-9 keV and abundances similar to 0.1-0.3 solar. The spatial analysis yields clear evidence that this emission is extended in NGC 253, and possibly also in M82. This quite clearly rules out a LLAGN as the main responsible for their hard X-ray emission. Significant contribution from point-sources (i.e. X-ray binaries (XRBs) and Supernovae Remnants (SNRs)) cannot be excluded; neither can we at present reliably estimate the level of Compton emission. However, we argue that such contributions shouldn't affect our main conclusion, i.e., that the BeppoSAX results show, altogether, compelling evidence for the existence of a, very hot, metal-poor interstellar plasma in both galaxies. (C) 1999 COSPAR. Published by Elsevier Science Ltd.
Diffuse thermal emission from very hot gas in starburst galaxies: Spatial results / Cappi, M; Persic, M; Mariani, S; Bassani, L; Danese, Luigi; Dean, Aj; Di Cocco, G; Franceschini, A; Hunt, Lk; Matteucci, F; Molendi, S; Palazzi, E; Palumbo, Ggc; Rephaeli, Y; Salucci, Paolo; Spizzichino, A.. - In: ADVANCES IN SPACE RESEARCH. - ISSN 0273-1177. - 23:5/6(1999), pp. 905-909. [10.1016/S0273-1177(99)00230-6]
Diffuse thermal emission from very hot gas in starburst galaxies: Spatial results
Danese, Luigi;Salucci, Paolo;
1999-01-01
Abstract
New BeppoSAX observations of the nearby prototypical starburst galaxies NGC 253 and M82 are presented. A companion paper (Cappi et al. 1998) shows that the hard (2-19 keV) spectrum of both galaxies, extracted from the source central regions, is best described by a thermal emission model with kT similar to 6-9 keV and abundances similar to 0.1-0.3 solar. The spatial analysis yields clear evidence that this emission is extended in NGC 253, and possibly also in M82. This quite clearly rules out a LLAGN as the main responsible for their hard X-ray emission. Significant contribution from point-sources (i.e. X-ray binaries (XRBs) and Supernovae Remnants (SNRs)) cannot be excluded; neither can we at present reliably estimate the level of Compton emission. However, we argue that such contributions shouldn't affect our main conclusion, i.e., that the BeppoSAX results show, altogether, compelling evidence for the existence of a, very hot, metal-poor interstellar plasma in both galaxies. (C) 1999 COSPAR. Published by Elsevier Science Ltd.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
