At infrared wavelengths, the ISM glows with blackbody radiation emitted by the interstellar dust.
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Q2: The composition of the interstellar dust suggests
Q3: Calculations of the Sun's future evolution indicate
Q6: The emission lines from O III are
Q8: Stars are born from the interstellar medium,
Q9: Molecular clouds are mapped using _ gas
Q9: H I clouds can be observed using
Q13: The interstellar medium is composed of mainly
Q14: Stars are born in reflection nebulae.
Q18: Elements such as carbon, silicon and oxygen
Q20: The ground state of hydrogen has two
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