C2H2 and HCN toward massive YSO's

Details C2H2 and HCN toward massive YSO's C2H2 and HCN toward massive YSO's

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000esasp.456..107l&link_type=abstract

ISO beyond the peaks: The 2nd ISO workshop on analytical spectroscopy. Eds. A. Salama, M.F.Kessler, K. Leech & B. Schulz. ESA-SP

Computer Science

Ism: Molecules, Methods: Data Analysis, Stars: Formation

Scientific paper

Observations of the ν5 vibration-rotation band of C2H2 around 13.7 μm and the ν2 band of HCN around 14.0 μm along the line of sight toward a large sample of deeply embedded massive young stellar objects (YSOs) have been made. The observed spectra and the inferred excitation temperatures, column densities, derived by comparison with model spectra, and the corresponding abundances are presented here. This paper summarises the poster presented at the conference. The published text with the complete results and full discussion can be found in Lahuis and van Dishoeck (2000).

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