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| | HISA Poster the 193rd Meeting of the AAS, January, 1999 |
 | | The ~2 kpc distance to the Perseus feature is based on the sightline velocity model of Roberts (1972), while the 200-500 pc distance for the Local feature is constrained merely to lie within the Local Arm, but outside the Local Bubble. |
 | | Instead, the peak in integrated opacity suggests a substantial abundance in HISA in the Perseus Arm, in full agreement with visual impressions of the amount of HISA in different channels of the velocity cube. |
 | | Figure 3 (Upper Left): Close-up of a HISA complex in the Perseus Arm at -41 km/s, with brightness ranging from 50-135 K. Yellow CO contours (Heyer et al.) are at 1, 3, and 5 K, and red 60 µm contours (Cao et al.) are at 15, 17, and 19 MJy/sr. |
| www.naic.edu /~gibson/hisa/poster/1999 (2005 words) |
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