Determining the origin of inner planetary system debris orbiting the dustiest main sequence stars

Carl Melis; B. Zuckerman; Joseph H. Rhee; Inseok Song; S. J. Murphy; M. S. Bessell

doi:10.1017/S1743921313012970

Determining the origin of inner planetary system debris orbiting the dustiest main sequence stars

Carl Melis, B. Zuckerman, Joseph H. Rhee, Inseok Song, S. J. Murphy, M. S. Bessell

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Abstract

We develop a means to distinguish between warm dusty circumstellar debris disks produced by steady state collisional evolution of a planetesimal belt or through transient events.

Original language	English
Title of host publication	Formation, Detection, and Characterization of Extrasolar Habitable Planets
Publisher	Cambridge University Press
Pages	273-277
Number of pages	5
Edition	S293
ISBN (Print)	9781107033825
DOIs	https://doi.org/10.1017/S1743921313012970
Publication status	Published - Aug 2012

Publication series

Name	Proceedings of the International Astronomical Union
Number	S293
Volume	8
ISSN (Print)	1743-9213
ISSN (Electronic)	1743-9221

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10.1017/S1743921313012970

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Melis, C., Zuckerman, B., Rhee, J. H., Song, I., Murphy, S. J., & Bessell, M. S. (2012). Determining the origin of inner planetary system debris orbiting the dustiest main sequence stars. In Formation, Detection, and Characterization of Extrasolar Habitable Planets (S293 ed., pp. 273-277). (Proceedings of the International Astronomical Union; Vol. 8, No. S293). Cambridge University Press. https://doi.org/10.1017/S1743921313012970

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title = "Determining the origin of inner planetary system debris orbiting the dustiest main sequence stars",

abstract = "We develop a means to distinguish between warm dusty circumstellar debris disks produced by steady state collisional evolution of a planetesimal belt or through transient events.",

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author = "Carl Melis and B. Zuckerman and Rhee, {Joseph H.} and Inseok Song and Murphy, {S. J.} and Bessell, {M. S.}",

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Melis, C, Zuckerman, B, Rhee, JH, Song, I, Murphy, SJ & Bessell, MS 2012, Determining the origin of inner planetary system debris orbiting the dustiest main sequence stars. in Formation, Detection, and Characterization of Extrasolar Habitable Planets. S293 edn, Proceedings of the International Astronomical Union, no. S293, vol. 8, Cambridge University Press, pp. 273-277. https://doi.org/10.1017/S1743921313012970

Determining the origin of inner planetary system debris orbiting the dustiest main sequence stars. / Melis, Carl; Zuckerman, B.; Rhee, Joseph H. et al.
Formation, Detection, and Characterization of Extrasolar Habitable Planets. S293. ed. Cambridge University Press, 2012. p. 273-277 (Proceedings of the International Astronomical Union; Vol. 8, No. S293).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

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Melis C, Zuckerman B, Rhee JH, Song I, Murphy SJ, Bessell MS. Determining the origin of inner planetary system debris orbiting the dustiest main sequence stars. In Formation, Detection, and Characterization of Extrasolar Habitable Planets. S293 ed. Cambridge University Press. 2012. p. 273-277. (Proceedings of the International Astronomical Union; S293). doi: 10.1017/S1743921313012970

Determining the origin of inner planetary system debris orbiting the dustiest main sequence stars

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