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Dust in HII Regions

  • Syuzo Isobe
Chapter
Part of the Astrophysics and Space Science Library book series (ASSL, volume 70)

Abstract

Several pieces of evidence indicate that HII regions may contain dust: 1) the continuum light scattered by dust grains (O’Dell and Hubbard, 1965),2) thermal radiation from dust grains at infrared wavelengths (Ney and Allen, 1969), 3) the abnormal helium abundance in some HII regions (Peimbert and Costero, 1969), etc.

Although observations of the scattered continuum suggest that the HII region cores may be dust-free, dust grains and gas must be well-mixed in view of the infrared observations. This difficulty may be solved by introducing globules with sizes ~0.001 pc. These globules and the molecular clouds adjacent to HII regions are the main sources supplying dust to HII regions.

Keywords

Molecular Cloud Column Density Surface Brightness Recombination Line Radio Observation 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing Company, Dordrecht, Holland 1977

Authors and Affiliations

  • Syuzo Isobe
    • 1
  1. 1.Tokyo Astronomical ObservatoryUniversity of TokyoMitaka, TokyoJapan

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