Inner part observation of the β pictoris disk

R. Ferlet; A. Lecavelier Des Etangs; G. Perrin; A. Vidal-Madjar; F. Sèvre; F. Colas; J. E. Arlot; C. Buil; H. Beust; A. M. Lagrange-Henri; J. Lecacheux; M. Deleuil; C. Gry

doi:10.1007/BF00984521

Inner part observation of the β pictoris disk

R. Ferlet
, A. Lecavelier Des Etangs
, G. Perrin
, A. Vidal-Madjar
, F. Sèvre
, F. Colas
, J. E. Arlot
, C. Buil
, H. Beust
, A. M. Lagrange-Henri
, J. Lecacheux
, M. Deleuil
, C. Gry

École Polytechnique

CNRS
Bureau des Longitudes
Centre National d'études Spatiales
Université Paris-Diderot
Groupe d'Astrophysique de Grenoble
LTHE (UMR 5564 CNRS/IRD/Université de Grenoble)
Laboratoire Univers et Theories (LUTH)
Sorbonne Univ.

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

2 Citations (Scopus)

Résumé

The inner regions of the circumstellar disk around β Pictoris might be dust-free due to a possible planet which may have cleared up dust particles. We present a new observational technique based on the use of an anti-blooming CCD in order to directly image this zone. The structure of the disk is revealed down to 2 arcsec from the star (30 AU). We show that the β Pic disk brightness is neutral in V, R, and I_C, but drops down when going inward in B, possibly related to a change in the dust composition. Also, a slight disk asymmetry is present but inverted from the outer to the inner zones.

langue originale	Anglais
Pages (de - à)	173-180
Nombre de pages	8
journal	Astrophysics and Space Science
Volume	212
Numéro de publication	1-2
Les DOIs	https://doi.org/10.1007/BF00984521
état	Publié - 1 févr. 1994

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10.1007/BF00984521

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@article{bdc4842393a942f8a2b357b808440811,

title = "Inner part observation of the β pictoris disk",

abstract = "The inner regions of the circumstellar disk around β Pictoris might be dust-free due to a possible planet which may have cleared up dust particles. We present a new observational technique based on the use of an anti-blooming CCD in order to directly image this zone. The structure of the disk is revealed down to 2 arcsec from the star (30 AU). We show that the β Pic disk brightness is neutral in V, R, and IC, but drops down when going inward in B, possibly related to a change in the dust composition. Also, a slight disk asymmetry is present but inverted from the outer to the inner zones.",

author = "R. Ferlet and \{Lecavelier Des Etangs\}, A. and G. Perrin and A. Vidal-Madjar and F. S{\`e}vre and F. Colas and Arlot, \{J. E.\} and C. Buil and H. Beust and Lagrange-Henri, \{A. M.\} and J. Lecacheux and M. Deleuil and C. Gry",

year = "1994",

month = feb,

day = "1",

doi = "10.1007/BF00984521",

language = "English",

volume = "212",

pages = "173--180",

journal = "Astrophysics and Space Science",

issn = "0004-640X",

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}

TY - JOUR

T1 - Inner part observation of the β pictoris disk

AU - Ferlet, R.

AU - Lecavelier Des Etangs, A.

AU - Perrin, G.

AU - Vidal-Madjar, A.

AU - Sèvre, F.

AU - Colas, F.

AU - Arlot, J. E.

AU - Buil, C.

AU - Beust, H.

AU - Lagrange-Henri, A. M.

AU - Lecacheux, J.

AU - Deleuil, M.

AU - Gry, C.

PY - 1994/2/1

Y1 - 1994/2/1

N2 - The inner regions of the circumstellar disk around β Pictoris might be dust-free due to a possible planet which may have cleared up dust particles. We present a new observational technique based on the use of an anti-blooming CCD in order to directly image this zone. The structure of the disk is revealed down to 2 arcsec from the star (30 AU). We show that the β Pic disk brightness is neutral in V, R, and IC, but drops down when going inward in B, possibly related to a change in the dust composition. Also, a slight disk asymmetry is present but inverted from the outer to the inner zones.

AB - The inner regions of the circumstellar disk around β Pictoris might be dust-free due to a possible planet which may have cleared up dust particles. We present a new observational technique based on the use of an anti-blooming CCD in order to directly image this zone. The structure of the disk is revealed down to 2 arcsec from the star (30 AU). We show that the β Pic disk brightness is neutral in V, R, and IC, but drops down when going inward in B, possibly related to a change in the dust composition. Also, a slight disk asymmetry is present but inverted from the outer to the inner zones.

U2 - 10.1007/BF00984521

DO - 10.1007/BF00984521

M3 - Article

AN - SCOPUS:34249773877

SN - 0004-640X

VL - 212

SP - 173

EP - 180

JO - Astrophysics and Space Science

JF - Astrophysics and Space Science

IS - 1-2

ER -

Inner part observation of the β pictoris disk

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