z-logo
open-access-imgOpen Access
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

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom