FileTitleManuscript Id
[Unknown Title]universe10e_ch20_1.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_1_dlap.xml534c6b8d757a2e4930000002
20-1 Stars of between 0.4 and 4 solar masses go through two distinct red giant stages universe10e_ch20_2.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_2_dlap.xml534c6b8d757a2e4930000002
20-2 Dredge-ups bring the products of nuclear fusion to a giant star’s surface universe10e_ch20_3.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_3_dlap.xml534c6b8d757a2e4930000002
20-3 Stars of moderately low mass die by gently ejecting their outer layers, creating planetary nebulae universe10e_ch20_4.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_4_dlap.xml534c6b8d757a2e4930000002
20-4 The burned-out core of a moderately low-mass star cools and contracts until it becomes a white dwarf universe10e_ch20_5.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_5_dlap.xml534c6b8d757a2e4930000002
20-5 High-mass stars create heavy elements in their cores universe10e_ch20_6.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_6_dlap.xml534c6b8d757a2e4930000002
20-6 High-mass stars violently blow apart in core-collapse supernova explosions universe10e_ch20_7.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_7_dlap.xml534c6b8d757a2e4930000002
20-7 In 1987 a nearby supernova gave us a close-up look at the death of a massive star universe10e_ch20_8.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_8_dlap.xml534c6b8d757a2e4930000002
20-8 Neutrinos emanate from supernovae like SN 1987A universe10e_ch20_9.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_9_dlap.xml534c6b8d757a2e4930000002
20-9 White dwarfs in close binary systems can also become supernovae universe10e_ch20_10.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_10_dlap.xml534c6b8d757a2e4930000002
20-10 A supernova remnant can be detected at many wavelengths for centuries after the explosion universe10e_ch20_11.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_11_dlap.xml534c6b8d757a2e4930000002
20-11 Neutron stars universe10e_ch20_12.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_12_dlap.xml534c6b8d757a2e4930000002
20-12 Explosive nuclear processes on white dwarfs and neutron stars produce novae and bursters universe10e_ch20_13.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_13_dlap.xml534c6b8d757a2e4930000002
Key Wordsuniverse10e_ch20_14.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_14_dlap.xml534c6b8d757a2e4930000002
Key Ideasuniverse10e_ch20_15.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_15_dlap.xml534c6b8d757a2e4930000002
Questionsuniverse10e_ch20_16.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_16_dlap.xml534c6b8d757a2e4930000002
Activitiesuniverse10e_ch20_17.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_17_dlap.xml534c6b8d757a2e4930000002
Answersuniverse10e_ch20_18.html534c6b8d757a2e4930000002
DLAP questionsuniverse10e_ch20_18_dlap.xml534c6b8d757a2e4930000002