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slater2e_ch11_1.html53922a72757a2e4848000003
DLAP questionsslater2e_ch11_1_dlap.xml53922a72757a2e4848000003
11-1 Stars form from the gravitational collapse of immense clouds of interstellar gas and dust slater2e_ch11_2.html53922a72757a2e4848000003
DLAP questionsslater2e_ch11_2_dlap.xml53922a72757a2e4848000003
11-2 Most stars shine throughout their lives by converting hydrogen into helium through nuclear fusion slater2e_ch11_3.html53922a72757a2e4848000003
DLAP questionsslater2e_ch11_3_dlap.xml53922a72757a2e4848000003
11-3 Careful observations of star clusters provide insight into how a star’s mass influences how stars change over time slater2e_ch11_4.html53922a72757a2e4848000003
DLAP questionsslater2e_ch11_4_dlap.xml53922a72757a2e4848000003
11-4 Stars slowly become red giants slater2e_ch11_5.html53922a72757a2e4848000003
DLAP questionsslater2e_ch11_5_dlap.xml53922a72757a2e4848000003
11-5 Low-mass stars pulsate and eject planetary nebulae, leaving behind a white dwarf at the end of their life cycles slater2e_ch11_6.html53922a72757a2e4848000003
DLAP questionsslater2e_ch11_6_dlap.xml53922a72757a2e4848000003
Key Ideas and Termsslater2e_ch11_7.html53922a72757a2e4848000003
DLAP questionsslater2e_ch11_7_dlap.xml53922a72757a2e4848000003
Questionsslater2e_ch11_8.html53922a72757a2e4848000003
DLAP questionsslater2e_ch11_8_dlap.xml53922a72757a2e4848000003
Answersslater2e_ch11_9.html53922a72757a2e4848000003
DLAP questionsslater2e_ch11_9_dlap.xml53922a72757a2e4848000003