A Comparison between Anomalous 6 cm H sub(2)CO Absorption and CO(1-0) Emission in the L1204/S140 Region

We report observations of the dust cloud L1204 with the Onsala 25 m telescope in the 6 cm (1 sub(11)-1 sub(10)) transition of H sub(2)CO. The observed region includes the S140 Ho arc. This spectral line is seen here in absorption against the cosmic microwave background, indicating the presence of widespread warm molecular gas at intermediate densities. Overall, the distributions of H sub(2)CO and CO (taken from the literature) are fairly similar, although significant differences exist at small scales. Most notably, While the CO peak is nearly coincident with the S140 Ho arc, the maximum H sub(2)CO absorption is clearly separated from it by a full 10' beam ( similar to 3 pc). We argue that these differences result from differing abundances and excitation requirements. The CO(1-0) line is more optically thick and more biased toward warm gas than the H sub(2)CO 6 cm line. On the other hand, formaldehyde is more easily photodissociated and is, therefore, a poorer tracer of the molecular gas located immediately behind photon-dominated regions.