PRIMORDIAL LIH - THE CHEMISTRY IN A COLLAPSING PROTOCLOUD

Authors
Citation
D. Puy et M. Signore, PRIMORDIAL LIH - THE CHEMISTRY IN A COLLAPSING PROTOCLOUD, New astronomy, 3(1), 1997, pp. 27-36
Citations number
36
Journal title
ISSN journal
13841092
Volume
3
Issue
1
Year of publication
1997
Pages
27 - 36
Database
ISI
SICI code
1384-1092(1997)3:1<27:PL-TCI>2.0.ZU;2-9
Abstract
We analyse and discuss the evolution of primordial molecules during th e beginning stage of the early cloud formation using an updated primor dial lithium chemistry. As Puy & Signore (1996)[A & A, 305, 371], (199 7)[NewA, 2, 299], we consider a simple model of a collapsing protoclou d after the recombination epoch but paying special attention to the Li H formation by radiative association from excited Li atoms. Because th e rate of LiH destruction through collisions with H atoms is only esti mated we find that, at present, the percentage of primordial lithium c onverted to LiH is quite uncertain. (C) 1998 Elsevier Science B.V.