colo/didattica/nucleare/nuclastro.pdf · 2010-01-26 · cools slowly and its luminosity decreases....

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Page 1: colo/Didattica/Nucleare/nuclastro.pdf · 2010-01-26 · cools slowly and its luminosity decreases. The star becomes a white dwarf some casæ its diameter can become smaller than that
Page 2: colo/Didattica/Nucleare/nuclastro.pdf · 2010-01-26 · cools slowly and its luminosity decreases. The star becomes a white dwarf some casæ its diameter can become smaller than that
Page 3: colo/Didattica/Nucleare/nuclastro.pdf · 2010-01-26 · cools slowly and its luminosity decreases. The star becomes a white dwarf some casæ its diameter can become smaller than that
Page 4: colo/Didattica/Nucleare/nuclastro.pdf · 2010-01-26 · cools slowly and its luminosity decreases. The star becomes a white dwarf some casæ its diameter can become smaller than that
Page 5: colo/Didattica/Nucleare/nuclastro.pdf · 2010-01-26 · cools slowly and its luminosity decreases. The star becomes a white dwarf some casæ its diameter can become smaller than that
Page 6: colo/Didattica/Nucleare/nuclastro.pdf · 2010-01-26 · cools slowly and its luminosity decreases. The star becomes a white dwarf some casæ its diameter can become smaller than that
Page 7: colo/Didattica/Nucleare/nuclastro.pdf · 2010-01-26 · cools slowly and its luminosity decreases. The star becomes a white dwarf some casæ its diameter can become smaller than that
Page 8: colo/Didattica/Nucleare/nuclastro.pdf · 2010-01-26 · cools slowly and its luminosity decreases. The star becomes a white dwarf some casæ its diameter can become smaller than that
Page 9: colo/Didattica/Nucleare/nuclastro.pdf · 2010-01-26 · cools slowly and its luminosity decreases. The star becomes a white dwarf some casæ its diameter can become smaller than that