The determination of cloud masses and dust characteristics from submillimeter thermal emission

  • Hildebrand R
  • 85

    Readers

    Mendeley users who have this article in their library.
  • N/A

    Citations

    Citations of this article.

Abstract

The purpose of this paper is to review the principles by which the dust masses and total masses of interstellar clouds and certain characteristics of interstellar dust grains can be derived from observations of far-infrared and submillimetre thermal emission. To the extent possible, the discussion will be independent of particular grain models.

Author-supplied keywords

  • icle

Get free article suggestions today

Mendeley saves you time finding and organizing research

Sign up here
Already have an account ?Sign in

Find this document

Authors

  • Roger H. Hildebrand

Cite this document

Choose a citation style from the tabs below

Save time finding and organizing research with Mendeley

Sign up for free