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Extrasolar comets

  • Institut d’Astrophysique de Paris

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

Gaseous and dusty circumstellar disks are commonly thought to be the birth place of planetary systems. Once planets are formed, the so-called "debris disks" are still active complex evolving systems in which gas and dust are interacting and replenishing. This was notably demonstrated through visible and UV absorption spectroscopy of the most famous debris disk around the main sequence star β Pictoris. Hourly variable absorbing components are explained by a multitude of sublimating comets when grazing the star. This intense cometary activity is the proposed source for the gas and one possible origin for the replenishment of the dust. Hundreds of cometary-like events are observed, from different comet families.

Original languageEnglish
Title of host publicationPrecision Spectroscopy in Astrophysics
Subtitle of host publicationProceedings of the ESO/Lisbon/Aveiro Conference held in Aveiro, Portugal, 11-15 September 2006
EditorsNuno C. Santos, Luca Pasquini, Martino Romaniello, Alexandre C. M. Correia
Pages211-214
Number of pages4
DOIs
Publication statusPublished - 1 Jan 2008
Externally publishedYes

Publication series

NameESO Astrophysics Symposia
Volume2008
ISSN (Print)1431-2433
ISSN (Electronic)1611-6143

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