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casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio

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Page 1: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 2: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 3: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 4: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 5: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 6: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 7: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 8: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 9: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 10: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 11: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 12: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 13: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 14: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 15: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 16: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 17: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 18: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio
Page 19: casca.cacasca.ca/wp-content/uploads/2014/09/CAS85_1994_Dec.pdf · helium, persists at low effective temperatures. In particular, no white dwarf star with a helium-to-hydrogen ratio

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