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Ammonia absorption toward NGC 7538 IRS 1: 2 ARC second observations in the (3,3) line

Journal Article · · Astrophys. J., Lett. Ed.; (United States)
DOI:https://doi.org/10.1086/184313· OSTI ID:6176036
Absorption from the (3,3) line of NH/sub 3/ has been detected at -60.0 km s/sup -1/ toward the ultracompact H II region IRS 1 in NGC 7538 with the VLA. In single-dish spectra, the line is blended with an emission component at -56.5 km s/sup -1/. With the 2.5 x 2.2 beam, however, line emission is resolved out. This corresponds to a spatial extent of more than 10''. The measured width of the absorption line is 8.5 km s/sup -1/ (FWHP). Accounting for the total optical depth of approximately 25 (estimated from hyperfine ratios), we obtain an intrinsic unsaturated line width of approximately 3.5 km s/sup -1/. The line shape appears not to be compatible with a single Gaussian-shaped velocity component of high optical depth. The molecular cloud covers at least 60% of the continuum source; this is approximately 1'', corresponding to 0.017 pc. From the line shape, the cloud may consist of several clumps of size less than 0.01 pc, each with a different radial velocity and smaller line width. In addition to the spectral line measurements, a 23.87 GHz continuum map of IRS 1, 2, 3 is presented. The electron density in IRS 1 is found to be roughly 2 x 10/sup 5/ cm/sup -3/. It is suggested that IRS 1 and IRS 2 may be similar objects at a different state of their evolution.
Research Organization:
Max-Planck-Institut fuer Radioastronomie, Bonn, Federal Republic of Germany
OSTI ID:
6176036
Journal Information:
Astrophys. J., Lett. Ed.; (United States), Journal Name: Astrophys. J., Lett. Ed.; (United States) Vol. 282:2; ISSN AJLEA
Country of Publication:
United States
Language:
English