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A review of the first observations of stars using the Infrared Astronomical Satellite (IRAS)

  • 3. Results from the Infrared Astronomical Satellite
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Cool Stars, Stellar Systems, and the Sun

Part of the book series: Lecture Notes in Physics ((LNP,volume 193))

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Abstract

The primary aim of the IRAS mission is a survey of the entire sky at infrared wavelengths of 12, 25, 60 and 100 μm. Some of the preliminary results of the IRAS mission relating to stars include: 1) a characterization of the properties of the infrared sky based on a careful survey of a 900 sq. dog. of sky; 2) the presence of young stars of roughly solar mass within the dense cores of dark clouds; 3) the existence of a cloud of large dust particles around the AO V star, Vega, implying, perhaps, the existence of a pre-planetary system around that star; and 4) the discovery of the infrared counterparts to a large number of stellar OH masers.

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Sallie L. Baliunas Lee Hartmann

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© 1984 Springer-Verlag

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Beichman, C.A. et al. (1984). A review of the first observations of stars using the Infrared Astronomical Satellite (IRAS). In: Baliunas, S.L., Hartmann, L. (eds) Cool Stars, Stellar Systems, and the Sun. Lecture Notes in Physics, vol 193. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-12907-3_209

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  • DOI: https://doi.org/10.1007/3-540-12907-3_209

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