Green 1994
Green, S., 1994: Collisional excitation of interstellar sulfur monoxide. Astrophys. J., 434, 188-191, doi:10.1086/174715.
Excitation rates among fine structure levels of sulfur monoxide in collisions with hydrogen molecules are estimated using methods expected to provide adequate accuracy for modeling millimeter and submillimeter observations of this species in relatively warm (100-300 K) molecular clouds.
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Green, S.: Collisional excitation of interstellar sulfur monoxide, Astrophys. J., 434, 188-191, doi:10.1086/174715, 1994.
Green, S. (1994), Collisional excitation of interstellar sulfur monoxide, Astrophys. J., 434, 188-191, doi:10.1086/174715.
Green, S., 1994: Collisional excitation of interstellar sulfur monoxide. Astrophys. J., 434, 188-191, doi:10.1086/174715.
Green, S. 1994, Astrophys. J., 434, 188, doi:10.1086/174715.
Green S. Collisional excitation of interstellar sulfur monoxide, Astrophys J 1994;434:188-191. doi:10.1086/174715.
S. Green, Astrophys. J. 434, 188-191, doi:10.1086/174715 (1994).
