Co and C 2 Absorption toward W40 Irs 1a

The H II region W40 harbors a small group of young, hot stars behind roughly 9 magnitudes of visual extinction. We have detected gaseous carbon monoxide (CO) and diatomic carbon (C2) in absorption toward the star W 40 IRS 1a. The 2-0 R0, R1, and R2 lines of 12CO at 2.3 μm were measured using the CSHELL on the NASA IR Telescope Facility (with upper limits placed on R3, R4, and R5) yielding an NCO of (1.1 ± 0.2) × 10 18 cm−2. Excitation analysis indicates Tkin > 7 K. The Phillips system of C2 transitions near 8775 Å was measured using the Kitt Peak 4-m telescope and echelle spectrometer. Radiative pumping models indicate a total C2 column density of (7.0 ± 0.4) × 10 14 cm−2, two excitation temperatures (39 and 126 K), and a total gas density of n ∼ 250 cm−3. The CO ice band at 4.7 μm was not detected, placing an upper limit on the CO depletion of δ < 1%. We postulate that the sightline has multiple translucent components and is associated with the W40 molecular cloud. Our data for W40 IRS 1a coupled with other sightlines, shows that the ratio of CO/C2 increases from diffuse through translucent environs. Finally, we show that the hydrogen to dust ratio seems to remain constant from diffuse to dense environments, while the CO to dust ratio apparently does not. Subject headings: dust, extinction – infrared: ISM: lines and bands — ISM: abundances — ISM: clouds — ISM: individual (W40) — ISM: molecules