2006ApJ...636..908G -
Astrophys. J., 636, 908-915 (2006/January-2)
Molecular hydrogen in infrared cirrus.
GILLMON K. and SHULL J.M.
Abstract (from CDS):
We combine data from our recent FUSE survey of interstellar molecular hydrogen absorption toward 50 high-latitude AGNs with COBE-corrected IRAS 100 µm emission maps to study the correlation of infrared cirrus with H2. A plot of the H2column density versus IR cirrus intensity shows the same transition in molecular fraction, fH2, as seen with total hydrogen column density, NH. This transition is usually attributed to H2 ``self-shielding'', and it suggests that many diffuse cirrus clouds contain H2in significant fractions, fH2~1%-30%. These clouds cover ∼50% of the northern sky at b>30°, at temperature-corrected 100 µm intensities DT100≥1.5 MJy/sr. The sheetlike cirrus clouds, with hydrogen densities nH≥30/cm3, may be compressed by dynamical processes at the disk-halo interface, and they are conducive to H2formation on grain surfaces. Exploiting the correlation between NH2and 100 µm intensity, we estimate that cirrus clouds at b>30° contain ∼3000 M☉in H2. Extrapolated over the inner Milky Way, the cirrus may contain 107 M☉of H2and 108 M☉in total gas mass. If elevated to 100 pc, their gravitational potential energy is ∼1053 ergs.
Abstract Copyright:
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Journal keyword(s):
ISM: Dust, Extinction - Infrared: ISM - ISM: Clouds - ISM: Molecules - Ultraviolet: ISM
Simbad objects:
20
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