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2013ApJ...776L..38F - Astrophys. J., 776, L38 (2013/October-3)
A significantly low CO abundance toward the TW Hya protoplanetary disk: a path to active carbon chemistry?
FAVRE C., CLEEVES L.I., BERGIN E.A., QI C. and BLAKE G.A.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): astrochemistry - ISM: abundances - protoplanetary disks - stars: formation
Simbad objects: 4
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