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Review of results in infrared space astronomy. (1972)

Hoffmann, W. F.

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Publication Date: 2019-07-13

Description: Some stars, in particular, T Tauri stars, have substantial IR excesses at 10 microns. It is now understood that the long wavelength radiation comes from a shell of dust which surrounds the star and absorbs the stellar radiation. Part of the mass which is lost from supergiants is condensed into solid particles which remain in the stellar environment and provide the excess IR radiation. The most intense far-infrared object outside the solar system is the galactic center. Diffuse galactic IR objects include extended regions of gas and dust surrounding very hot young stars and regions of gas and dust surrounding cooler stars. Other subjects considered include IR galaxies and cosmic radiation.

Keywords: SPACE SCIENCES

Type: ESLAB-ESRIN Symposium; Jun 08, 1971 - Jun 11, 1971; Noordwijk; Netherlands

Format: text

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