On the Spectral Distribution of Infrared Objects and Related Stars

Details On the Spectral Distribution of Infrared Objects and Related Stars On the Spectral Distribution of Infrared Objects and Related Stars

Jul 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970pthph..44...99m&link_type=abstract

Progress of Theoretical Physics, Vol. 44, No. 1, pp. 99-109

Physics

2

Scientific paper

The spectra of infrared stars and the anomalous excess emissions in the infrared region of T Tauri stars or some red giant stars are interpreted by an effect of circumstellar dust clouds. We have calculated a probable model of dust-stars assuming the distribution of dust particles in the circumstellar space including absorption, scattering and thermal re-emission processes by them. We can see that the spectra calculated by the use of a rather simple model of the circumstellar dust envelope well fit the infrared spectra observed so far by photometric measurement.

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