The spectra of the youngest stars show the most heavy elements present.
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Q9: Iron nuclei are the most tightly bound
Q10: Stellar nucleosynthesis is responsible for the existence
Q11: Novae are more closely related to Type
Q12: Iron is the most stably bonded atomic
Q13: A carbon-detonation supernova starts out as a
Q15: Unlike supernovae, novae can explode more than
Q16: Type II supernovae have little hydrogen in
Q17: Except for hydrogen and most of the
Q18: Because they all involve the detonation of
Q19: Most of the energy released during a
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