Titre du document

Some Implications of the Distribution of Interstellar Molecules

Lien vers le document
Nom du Corpus

AstroConcepts

Auteur(s)
  • Lewis E. Snyder Jr.
Affiliation(s)
  • Astronomy Dept., University of Virginia, 22903, Charlottesville, Va., USA
Résumé

It is suggested that molecular observations of interstellar clouds can be used to determine the stage of cloud evolution. However, before observational data can reliably be used to investigate the evolutionary path leading from a tenuous cloud of gas and interstellar dust to a star cluster, mechanisms of molecular formation, excitation, and destruction must be taken into account. The evidence is growing that interstellar dust grains have an important role in molecular formation and destruction.

Langue(s) du document
Anglais
Année de publication
1973
Revue

Interstellar Dust and Related Topics

Éditeur
Springer (e-books)
Type de publication
book-series
Type de document
research-article
Présence de XML structuré
Non
Version de PDF
1.4
Score de qualité du texte
6.489
Nom du concept
  • Astrochemistry
Identifiant ISTEX
D59A473C45AE6CCDD5B441858D7688D20FF7E8B0
ark:/67375/HCB-X96NK4HK-C
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