Journal
ASTROPHYSICAL JOURNAL
Volume 553, Issue 2, Pages L189-L191Publisher
UNIV CHICAGO PRESS
DOI: 10.1086/320686
Keywords
circumstellar matter; techniques : polarimetric
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Few circumstellar disks have been observed directly. Here we use sensitive differential polarimetric techniques to overcome atmospheric speckle noise in order to image the circumstellar material around HD 169142. The detected envelope or disk is considerably smaller than expectations based on the measured strength of the far-IR excess from this system.
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