Astronomical detection of rhomboidal SiC3

Citation
Aj. Apponi et al., Astronomical detection of rhomboidal SiC3, ASTROPHYS J, 516(2), 1999, pp. L103-L106
Citations number
14
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICAL JOURNAL
ISSN journal
0004637X → ACNP
Volume
516
Issue
2
Year of publication
1999
Part
2
Pages
L103 - L106
Database
ISI
SICI code
0004-637X(19990510)516:2<L103:ADORS>2.0.ZU;2-G
Abstract
Seven rotational transitions of SIG,, a planar, highly polar ring molecule, have been detected in the millimeterwave band in the expanding envelope of the evolved carbon star IRC + 10216. On the assumption that SiC3 has: the same 40 " diameter shell as SiCC, the mean column density of SiC3 is 4.3 x 10(12) cm(-2). The rotational excitation of SiC3 is similar to that of SiCC , with a low rotational temperature within the K-stacks of 10-20 K and a hi gh rotational temperature across the K-stacks of roughly 50 K, which is pro bably close to the kinetic temperature of the shell.