Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.280..863c&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 280, Issue 3, pp. 863-867.
Astronomy and Astrophysics
Astronomy
7
Line: Profiles, Stars: Individual: Zeta Oph, Stars: Individual: Hd 169454, Ism: Molecules
Scientific paper
We have used the Ultra-High-Resolution Facility at the Anglo-Australian Telescope (AAT), operating at a resolution of 0.35 km s^-1 (FWHM), to measure the intrinsic profiles of the Q(2) and Q(4) lines of the (2-0) Phillips band of interstellar C_2 towards zeta Oph and HD 169454. The C_2 lines were found to be very narrow, with intrinsic velocity dispersions (b-values) in the range 0.25-0.71 km s^-1. In the case of zeta Oph, two velocity components (separation 1.10+/-0.17 km s^-1) have been resolved, and found to have rather different linewidths and rotational excitation temperatures. In the case of HD 169454, the data are consistent with a single velocity component, but the well-defined b-value (0.59+/-0.04 km s^-1) and low kinetic temperature would then imply supersonic turbulent velocities. One way to avoid this conclusion is to postulate the existence of unresolved velocity structure (or a velocity gradient) within the cloud.
Barlow Michael J.
Crawford Ian A.
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