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

Research output: Contribution to journalArticlepeer-review

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.

Original languageEnglish
Pages (from-to)173-180
Number of pages8
JournalAstrophysics and Space Science
Volume212
Issue number1-2
DOIs
Publication statusPublished - 1 Feb 1994

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