... II ] emission is excited by shocks in supernovaremnants (SNR) in the star-forming ... as the Orion Nebula) to an increasing r?le of shock excitation by supernovaremnants ...
... For M82, there is intense activity apparently leading to the large number of supernovaremnants (SNRs). ... Superconductor (a low noise microwave mixer) SNR -- supernovaremnant 51 SWAS -- Submillimeter Wave Astronomy Satellite VO ...
[
Текст
]
Ссылки http://www.stecf.org/coordination/esa_eso/alma-herschel/report.pdf -- 1000.5 Кб -- 04.09.2008 Похожие документы
... For stars and supernovaremnants we used Raymond-Smith models with energies of kT =0.5-2 keV, for X-ray binaries powerlaw ... for galaxies (warm and hot plasma mixture, powerlaw like emission from X-ray binaries, typical supernovaremnant spectra, etc ...
[
Текст
]
Ссылки http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/szokoly04.ps -- 1186.7 Кб -- 16.09.2004 Похожие документы
... stars and the short lifetimes of supernovaremnants mean such ob jects are not ... Supernovaremnants as tracers of present-day star formation rate lower the threshold ...
[
Текст
]
Ссылки http://www.stecf.org/coordination/esa_eso/galpops/report.pdf -- 2038.4 Кб -- 04.09.2008 Похожие документы