paper

The Relationship Between the Dust and Gas-Phase CO Across the California Molecular Cloud

arXiv:1503.03564 · doi:10.1088/0004-637X/805/1/58

Abstract

A deep, wide-field, near-infrared imaging survey was used to construct an extinction map of the southeastern part of the California Molecular Cloud (CMC) with 0.5 arc min resolution. The same region was also surveyed in the CO(2-1), CO(2-1), CO(2-1) emission lines at the same angular resolution. Strong spatial variations in the abundances of CO and CO were found to be correlated with variations in gas temperature, consistent with temperature dependent CO depletion/desorption on dust grains. The CO to CO abundance ratio was found to increase with decreasing extinction, suggesting selective photodissociation of CO by the ambient UV radiation field. The cloud averaged X-factor is found to be X 2.53 10 , somewhat higher than the Milky Way average. On sub-parsec scales we find no single empirical value of the X-factor that can characterize the molecular gas in cold (T 15 K) regions, with X A for A 3 magnitudes. However in regions containing relatively hot (T 25 K) gas we find a clear correlation between W(CO) and A over a large (3 A 25 mag) extinction range. This suggests a constant X 1.5 10 for the hot gas, a lower value than either the average for the CMC or Milky Way. We find a correlation between X and T with X T suggesting that the global X-factor of a cloud may depend on the relative amounts of hot gas within it.

21 pages, 17 figures, accepted by ApJ