Methanol in the L1551 Circumbinary Torus
Author(s) -
G. J. White,
Cvm Fridlund,
P. Bergman,
A. Beardsmore,
René Liseau,
M. C. Price,
R. Phillips
Publication year - 2006
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/509570
Subject(s) - planetesimal , circumbinary planet , astrophysics , torus , physics , astronomy , stars , solar system , geometry , mathematics
We report observations of gaseous methanol in an edge-on torus surroundingthe young stellar object L1551 IRS5. The peaks in the torus are separated by ~10,000 AU from L1551 IRS5, and contain ~ 0.03 earth masses of cold methanol. Weinfer that the methanol abundance increases in the outer part of the torus,probably as a result of methanol evaporation from dust grain surfaces heated bythe shock luminosity associated with the shocks associated with the jets of anexternally located x-ray source. Any methanol released in such a coldenvironment will rapidly freeze again, spreading methanol throughout thecircumbinary torus to nascent dust grains, planitesimals, and primitive bodies.These observations probe the initial chemical conditions of matter infallingonto the disk.Comment: 5 pages four figures. ApJ Letters in pres
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