Water cooling of shocks in protostellar outflows: Herschel-PACS map of L1157

Autor: Nisini, B., Benedettini, M., Codella, C., Giannini, T., Liseau, R., Neufeld, D., Tafalla, M., van Dishoeck, E. F., Bachiller, R., Baaudry, A., Benz, O. A., Bergin, E., Bjerkeli, P., Blake, G., Bontemps, S., Braine, J., Bruderer, S., Caselli, P., Cernicharo, J., Daniel, F., Encrenaz, P., di Giorgio, A. M., Dominik, C., Doty, S., Fich, M., Fuente, A., Goicoechea, J. R., de Graaw, Th., Helmich, F., Herczeg, G., Herpin, F., Hogerheijde, M., Jacq, T., Johnstone, D., Jorgensen, J., Kaufman, M., Kirstensen, L., Larsson, B., Lis, D., Marseille, M., McCoey, C., Melnick, G., Olberg, M., Parise, B., Pearson, J., Plime, R., Risacher, C., Santiago, J., Saraceno, P., Shipman, R., van Kempen, T. A., Visser, R., Viti, S., Wampfler, S., Wyrowski, F., van der Tak, F., Yildiz, U. A., Delforge, B., Desbat, J., Hatch, W. A., Peron, I., Schieder, R., Stern, J. A., Teyssier, D., Whyborn, N.

In the framework of the Water in Star-forming regions with Herschel (WISH) key program, maps in water lines of several outflows from young stars are being obtained, to study the water production in shocks and its role in the outflow cooling. This pap

Externí odkaz: http://arxiv.org/abs/1005.4517