A Search for Warm Circumstellar Disks in the TW Hydrae Association
Author(s) -
Alycia J. Weinberger,
E. E. Becklin,
B. Zuckerman,
Inseok Song
Publication year - 2004
Publication title -
the astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.61
H-Index - 271
eISSN - 1538-3881
pISSN - 0004-6256
DOI - 10.1086/382519
Subject(s) - circumstellar dust , stars , physics , circumstellar disk , zodiacal light , photometry (optics) , astrophysics , planet , astronomy
A search for previously undetected optically thin disks around stars in thenearby, young, TW Hydrae Association was conducted around sixteen stars withsensitive 12 and 18 micron photometry. The survey could detect Zodiacal-likedust, with temperature 200-300 K, at levels of L(IR)/L(*)=7e-3. Possiblemid-infrared excess emission from TWA 17 was detected at the 2-sigma level, butnone of the other stars showed evidence for circumstellar dust. The rapiddisappearance of large amounts of dust around the K and M-type stars in thissample may mean that any planet formation in the terrestrial planet region wascompleted very quickly. There appears to be a bi-modal distribution of dustdisks in TWA with stars having either copious or negligible warm dust.Comment: Accepted to AJ for April 2004 issu
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom