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| Paper: |
CO and H2O models of the protostellar object B 335 |
| Volume: |
132, Star Formation with the Infrared Space Observatory (ISO) |
| Page: |
362 |
| Authors: |
Hartstein, Daniel; Liseau, Rene |
| Abstract: |
We use a Monte Carlo code capable of treating radiative transfer problems at high optical depths to predict rotational H2O line spectra for the protostellar object B 335, and compare these with {sc Iso}-observations. We also apply our model to line profiles of CO isotopomers for comparison with observations, and to derive the cooling rate for B 335. We find that the CO cooling rate is greater than the H2O cooling rate even for the highest water abundances. |
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