Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-24T11:14:34.600Z Has data issue: false hasContentIssue false

Distribution of Dust in the Disk Around Beta Pictoris

Published online by Cambridge University Press:  12 April 2016

Takenori Nakano*
Affiliation:
Nobeyama Radio Observatory, National Astronomical Observatory Nobeyama, Minamisaku, Nagano 384-13, Japan

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Large far-infrared excesses in some nearby main-sequence stars, revealed by the Infrared Astronomical Satellite (IRAS), have been interpreted as being due to thermal radiation from dust orbiting the stars, heated to about 100K by the stellar radiation (Aumann et al. 1984; Aumann 1985; Sadakane and Nishida 1986). The existence of solid circumstellar material is commonly interpreted in the context of planet formation, and the dust has been suggested to be formed by collisions of planetesimals (Nakano 1987, 1988).

Type
Origin of Interplanetary Dust: from Comets and Asteroids, Back to Interstellar Dust
Copyright
Copyright © Kluwer 1991

References

Artymowicz, P., Burrows, C., and Paresce, F., 1989, Asirophys. J., 337, 494.CrossRefGoogle Scholar
Aumann, H.H. 1985, Publ. Astr. Soc. Pacific, 97, 885.Google Scholar
Aumann, H.H., et al. 1984. Asirophys. J. (Leiiers), 278, L23.CrossRefGoogle Scholar
Backman, D.E., and Gillett, F.C. 1987, Cool Stars, Stellar Systems, and the Sun, ed. Linsky, J. L. and Stencel, R. E. (Berlin: Springer), p. 340.CrossRefGoogle Scholar
Buitrago, J., and Mediavilla, E. 1986. Asir. Asirophys., 162, 95.Google Scholar
Leinert, C., Link, H., Pitz, E., and Giese, R.H. 1976, Astr. Asirophys., 47, 221.Google Scholar
Leinert, C., Röser, S., and Buitrago, J. 1983, Astr. Astrophys., 118, 345.Google Scholar
Nakano, T. 1987, in IAU Symposium 115, Star Forming Regions, ed. Peimbert, M. and Jugaku, J. (Dordrecht: Reidel), p. 301.Google Scholar
Nakano, T. 1988, Mon. Not Roy. Asir. Soc., 230, 551.Google Scholar
Nakano, T. 1990, Astrophys. J. (Letters), 355, L43.CrossRefGoogle Scholar
Paresce, F., and Burrows, C. 1987, Astrophys. J. (Letters), 319, L23.Google Scholar
Sadakane, K., and Nishida, M. 1986, Publ. Asir. Soc. Pacific, 98, 685.Google Scholar
Smith, B.A., and Terrile, R.J. 1984, Science, 226, 1421.CrossRefGoogle ScholarPubMed