Small-scale structure of the circumstellar gas around the very young outflow-driving source L483-FIR

A remarkable young stellar object in L483 numbers among the fewer than a do zen known youngest protostars, those with "class 0" spectral energy distrib utions. We report high angular and spectral resolution images of bright NH3 (1.,1) and NH3(2,2) line emission arising from the molecular gas near this object. Along the ridge of dense gas traced by the NH, (1,1) emission there is a velocity gradient of similar to 4 km s(-1) pc(-1). We also report ima ges of dust emission at lambda 450 mu m and lambda 850 mu m The images corr espond well over scales of thousands of AU. Near the star, however, the amm onia map corresponds in detail more closely with an image taken at lambda 3 .4 mu m than to the submillimeter images in that absorption in the near inf rared corresponds to an emission deficit in the ammonia maps. In the region of the deficit, the ammonia (1,1) line displays high optical depths, and i ts velocity is blueshifted relative to nearby gas and to other molecular li nes emanating from the region. We offer a specific model incorporating infa ll from the surrounding core onto the region within 3000 AU of the protosta r.