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slater2e_ch12_1.html53922a9d757a2e4548000005
DLAP questionsslater2e_ch12_1_dlap.xml53922a9d757a2e4548000005
12-1 High-mass stars create heavy elements in their cores before violently blowing apart in supernova explosions, leaving behind remnants slater2e_ch12_2.html53922a9d757a2e4548000005
DLAP questionsslater2e_ch12_2_dlap.xml53922a9d757a2e4548000005
12-2 Core-collapse supernovae can leave behind remnants, neutron stars, and pulsars slater2e_ch12_3.html53922a9d757a2e4548000005
DLAP questionsslater2e_ch12_3_dlap.xml53922a9d757a2e4548000005
12-3 Black holes are created in the death throes of the most massive of stars slater2e_ch12_4.html53922a9d757a2e4548000005
DLAP questionsslater2e_ch12_4_dlap.xml53922a9d757a2e4548000005
12-4 Black holes cannot be seen directly slater2e_ch12_5.html53922a9d757a2e4548000005
DLAP questionsslater2e_ch12_5_dlap.xml53922a9d757a2e4548000005
12-5 White dwarfs and pulsars in close binary systems can become novae, bursters, and supernovae slater2e_ch12_6.html53922a9d757a2e4548000005
DLAP questionsslater2e_ch12_6_dlap.xml53922a9d757a2e4548000005
Key Ideas and Termsslater2e_ch12_7.html53922a9d757a2e4548000005
DLAP questionsslater2e_ch12_7_dlap.xml53922a9d757a2e4548000005
Questionsslater2e_ch12_8.html53922a9d757a2e4548000005
DLAP questionsslater2e_ch12_8_dlap.xml53922a9d757a2e4548000005
Answersslater2e_ch12_9.html53922a9d757a2e4548000005
DLAP questionsslater2e_ch12_9_dlap.xml53922a9d757a2e4548000005