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Dust Around Solar Mass Stars

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Abstract

The DEBRIS project is a search for infrared excess around Sun-like main sequence stars, and other types of stellar targets, using the Infrared Space Observatory. Some results, calibration issues, and changes to our original program are presented. Future platforms for advancing this project after the conclusion of the ISO mission are indicated.

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References

  • Klaas, U., Krüger, H., Heinrichsen, I., Heske, A., and Laureijs, R. (eds) 1994, ISOPHOT Observer's Manual, Version 3.1

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Authors and Affiliations

  1. Division of Astronomy and Astrophysics University of California, Los Angeles, Los Angeles, CA, 90095-1562

    E.E. Becklin, M. Silverstone, R. Chary, J. Hare & B. Zuckerman

  2. Division of Physics, Mathematics and Astronomy, California Institute of Technology, Mail Stop 105-24, Pasadena, CA, 91125

    C. Spangler & A. Sargent

Authors
  1. E.E. Becklin
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  2. M. Silverstone
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  3. R. Chary
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  4. J. Hare
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  5. B. Zuckerman
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  6. C. Spangler
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  7. A. Sargent
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Becklin, E., Silverstone, M., Chary, R. et al. Dust Around Solar Mass Stars. Astrophysics and Space Science 255, 113–118 (1997). https://doi.org/10.1023/A:1001119005084

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  • DOI: https://doi.org/10.1023/A:1001119005084

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