Answer:it is wrong answer
Explanation:estro man
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The answer is b
Explanation:
Answer:
The amount of energy required to break the ionic bonds in CaF2.
Stars born larger than 8 solar masses usually retain enough mass to undergo core collapse, with the resulting shock wave producing a Type Ib supernova (spectra without Hydrogen or Silicon lines, with Helium lines), a Type Ic supernova (without Hydrogen or Helium or Silicon lines) or a Type II supernova
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