Rl. Akeson et Je. Carlstrom, LIFETIMES OF ULTRACOMPACT H-II REGIONS - HIGH-RESOLUTION METHYL CYANIDE OBSERVATIONS, The Astrophysical journal, 470(1), 1996, pp. 528-536
We observed the dense molecular cores associated with two ultracompact
H II regions, G5.89+-0.4 and G34.3+0.2, in the J = 6-5 transitions of
CH3CN to probe the temperature and density of the gas. Simultaneously
, each region was observed in the J = 1-0 transition of a CO isotope t
o probe the molecular column density. The molecular cores are found to
have densities similar to 10(6) cm(-3) and kinetic temperatures of 90
and 250 K, respectively. We also find possible evidence for infall of
molecular gas toward the H II regions. The lifetime of the H II regio
n ultracompact phase is critically dependent on the properties of the
surrounding molecular gas. Based on the number of ultracompact H II re
gions versus the total number of O stars, it has been suggested that t
he lifetime of the ultracompact phase is inconsistent with spherical e
xpansion cofined only by the ambient medium. We show that for the mole
cular cloud parameters given above and including the effect of the she
ll of neutral material formed by the expansion, pressure confinement b
y the ambient medium may significantly increase the lifetime of the ul
tracompact phase of the H II regions.