Sublimation temperature of circumstellar dust particles and its importance for dust ring formation-Reference-Cited by-同舟云学术

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Sublimation temperature of circumstellar dust particles and its importance for dust ring formation

Published:2011-10 Issue:10 Volume:63 Page:1067-1075
ISSN:1343-8832
Container-title:Earth, Planets and Space
language:en
Short-container-title:Earth Planet Sp

Author:

Kobayashi Hiroshi,Kimura Hiroshi,Watanabe Sei-ichiro,Yamamoto Tetsuo,Müller Sebastian

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Geology

Link

http://link.springer.com/content/pdf/10.5047/eps.2011.03.012

Reference40 articles.

1. Absil, O. et al., Circumstellar material in the Vega inner system revealed by CHARA/FLUOR, Astron. Astrophys., 452, 237–244, 2006.

2. Absil, O. et al., A near-infrared interferometric survey of debris disc stars. II. CHARA/FLUOR observations of six early-type dwarfs, Astron. Astrophys., 487, 1041–1054, 2008.

3. Akeson, R. L. et al., Dust in the inner regions of debris disks around a stars, Astrophys. J., 691,1896–1908, 2009.

4. Belton, M. J. S., Dynamics of interplanetary dust, Science, 151, 35–44, 1966.

5. Benz, W. and E. Asphaug, Catastrophic disruptions revisited, Icarus, 142, 5–20, 1999.

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