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Comment: 6 pages, To appear in Proceedings of International Conference on Nuclear Data for Science and Technology 2007 (ND2007), Nice, France
Comment: 2 figures; requires LaTeX A&A class file; accepted for publication in Astron. Astrophys
Comment: 10 pages, 2 figures; A&A in press
Comment: LaTeX2e with iopart.cls, 84 pages, 19 figures (graphicx package), 374 updated references. Published in Reports on Progress in Physics, vol.62, pp. 395-464 (1999)
Comment: to appear in "Astronomy with Radioactivities" (MPE Report; Eds. R. Diehl and D. Hartmann). Proc. of workshop held in Tegernsee (Germany), Oct 1999
Comment: 9 pages, no figures; ASP Conference Series: "Astrophysical Ages and Time Scales"
Neutrinos are a messenger of extreme condition inside a supernova core and a new-born neutron star. Since current ground-based detectors have potential to detect ~10,000 neutrinos from supernova at the galactic center, they could tell us lots of important physics. It includes: explosion mechanism, shock wave propagation, core temperature, and gravitational binding energy, as well as neutrino properties as elementary particle. In addition to the galactic supernova neutrino burst, one can still learn about them with diffuse supernova neutrino background, which is also soon to be detected. We review current situation from both points of view, and discuss prospects for future neutrino astrophysics.
Comment: 164 pages, 98 figures, accepted for publication in Phys. Rep. higher-quality version available at http://www-astro.ulb.ac.be
Comment: 8 pages, 3 figures, Review talk at Nuclei in the Cosmos 2000, Aarhus, June 27 - July 1, 2000
Comment: 9 pages including 5 figures. Conference proceedings for "CNO in the Universe", St Luc, Switzerland, 10-14 September 2002 C. Charbonnel, D. Schaerer & G. Meynet (eds) ASP Conference Serie
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