Issue |
A&A
Volume 409, Number 1, October I 2003
|
|
---|---|---|
Page(s) | 347 - 359 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361:20030995 | |
Published online | 17 November 2003 |
The physico-chemical history of Falling Evaporating Bodies around β Pictoris: The sublimation of refractory material
1
Laboratoire d'Astrophysique de Grenoble, Université J. Fourier, BP 53, 38041 Grenoble Cedex 9, France
2
Laboratoire de Planetologie de Grenoble, Université J. Fourier, BP 53, 38041 Grenoble Cedex 9, France
Corresponding author: H. Beust, herve.beust@obs.ujf-grenoble.fr
Received:
20
December
2002
Accepted:
3
June
2003
Transient spectral redshifted absorption
events in the spectrum of β Pictoris (β Pic) have been attributed to
comet-like bodies falling toward the star (Falling Evaporating Bodies,
or FEB) and evaporating in its immediate vicinity. Dynamical models shows
that these bodies originate from circular orbits at AU. After an
eccentricity increase due to planetary perturbations, they end up as
star-grazers. The physics of the cloud generated by the body's
sublimation is highly influenced by the physico-chemical conditions
inside the body. Thus it is necessary to investigate the composition
and the behavior of the materials within the body in order to explain
the observed features. The physico-chemical evolution of the bodies
has been simulated during all the phases before and during their FEB
state. First the fluctuations in the gas production rates of volatile
solids in the first phase when the refractory materials have not yet
evaporated has been studied. Later on, the refractory crust of the
object evaporates even if the core still contains volatile
solids. The simulation then shows a phase lag between the production
rate of volatiles and of refractory materials during the periastron
passage. The influence of dynamical and physical parameters on the FEB
phenomenon are also investigated. We find that only a heterogenous
population of bodies can produce all the absorption features
that have been observed so far. These results are important for
the understanding of the FEB phenomenon and can lead to a revision of
the FEB sublimation model.
Key words: stars: individual: β Pic / methods: numerical / comets: general / stars: circumstellar matter / stars: planetary systems: formation
© ESO, 2003
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