Interstellar H2 in M 33 detected with FUSE

Abstract

Fuse spectra of the four brightest $\ion{H}{ii}$ regions in M 33 show absorption by interstellar gas in the Galaxy and in M 33. On three lines of sight molecular hydrogen in M 33 is detected. This is the first measurement of diffuse H 2 in absorption in a Local Group galaxy other than the Magellanic Clouds. A quantitative analysis is difficult because of the low signal to noise ratio and the systematic effects produced by having multiple objects in the Fuse aperture. We use the M 33 Fuse data to demonstrate in a more general manner the complexity of interpreting interstellar absorption line spectra towards multi-object background sources. We derive H 2 column densities of ≈ 10 16 to 10 17 cm -2 along 3 sight lines (NGC 588, NGC 592, NGC 595). Because of the systematic effects, these values most likely represent upper limits and the non-detection of H 2 towards NGC 604 does not exclude the existence of significant amounts of molecular gas along this sight line.