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pro vyhledávání: '"Me'gie, G."'
Autor:
Larsson, B., Liseau, R., Pagani, L., Bergman, P., Bernath, P., Biver, N., Black, J. H., Booth, R. S., Buat, V., Crovisier, J., Curry, C. L., Dahlgren, M., Encrenaz, P. J., Falgarone, E., Feldman, P. A., Fich, M., Flore'n, H. G., Fredrixon, M., Frisk, U., Gahm, G. F., Gerin, M., Hagstroem, M., Harju, J., Hasegawa, T., Hjalmarson, Aa., Horellou, C., Johansson, L. E. B., Justtanont, K., Klotz, A., Kyroelae, E., Kwok, S., Lecacheux, A., Liljestroem, T., Llewellyn, E. J., Lundin, S., Me'gie, G., Mitchell, G. F., Murtagh, D., Nordh, L. H., Nyman, L. -Aa., Olberg, M., Olofsson, A. O. H., Olofsson, G., Olofsson, H., Persson, G., Plume, R., Rickman, H., Ristorcelli, I., Rydbeck, G., Sandqvist, Aa., Sche'ele, F. v., Serra, G., Torchinsky, S., Tothill, N. F., Volk, K., Wiklind, T., Wilson, C. D., Winnberg, A., Witt, G.
Molecular oxygen, O2 has been expected historically to be an abundant component of the chemical species in molecular clouds and, as such, an important coolant of the dense interstellar medium. However, a number of attempts from both ground and from s
Externí odkaz:
http://arxiv.org/abs/astro-ph/0702474
