Oct 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005kbls.confe...5b&link_type=abstract
Presented at the KITP: Blackboard Lunch Series, Oct 10, 2005, Kavli Institute for Theoretical Physics, University of California,
Physics
Scientific paper
Using only chalk and one figure, I will derive the luminosity,lifetime,
and major properties of all stars and explain why theirultimate fate
(white dwarf, neutron star or black hole) depends ontheir mass. After
this event, you should be able to explain itto your family and friends.
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