Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aas...191.7501k&link_type=abstract
American Astronomical Society, 191st AAS Meeting, #75.01; Bulletin of the American Astronomical Society, Vol. 29, p.1327
Astronomy and Astrophysics
Astronomy
1
Scientific paper
We present first results of an HST and ISO program to determine the fine-scale distribution of dust in spirals. We use neighboring early-type galaxies as background light sources to measure dust extinction in the HST data. We contrast the cases of two spirals projected in front of E/S0 galaxies, AM1316-241 and AM0500-620, from B and I WFPC2 images. In the outer arms, we find no regions with tau_B > 1.5 even at a typical resolution of 50 pc. AM0500-620 shows dust lanes associated with interarm spurs, while there is essentially no interarm dust seen in AM1316-241. The arm dust in AM0500-620 is strongly concentrated to rather thin narrow lanes, extending at least as far out as the optically detected arms do, while the dust distribution in AM1316-241 is broad and strongly textured. Within the dust arms of AM0500-620, we find some features which differ substantially in spatially averaged selective-to-total extinction, which suggests that the dust clumping and averaged column density may sometimes be decoupled. ISOCAM images at 17mu are available for AM1316-241, in which the strong backlit dust lane is undetected as a warm dust source (though we do expect it as a statistical contributor to the overall 50-100mu ISOPHOT maps). In an additional pair, AM1318-432=NGC 5090/1, the strong backlit dust lane is detected as a mid-IR source, signifying embedded star formation. When far-IR ISOPHOT data are added, we expect to derive significant constraints on the entire spatial spectrum of dust clumping.
Keel William C.
White Raymond Edwin III
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