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Molecular cloud: Revision history

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25 January 2026

  • curprev 21:2121:21, 25 January 2026 DanteWashere talk contribs 674 bytes +674 Created page with "'''Molecular cloud''' is a dense region of the interstellar medium composed primarily of molecular hydrogen, along with dust and trace molecules. It is associated with low temperatures and high densities relative to surrounding space. Molecular clouds are discussed in astrophysics, galactic astronomy, and studies of star formation. == Status == Molecular clouds are observed through radio and infrared measurements, including molecular line emission and dust absorption...."
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