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pro vyhledávání: '"Serrano, E. O."'
Autor:
Gómez-Ruiz, A. I., Guzman-Ramirez, L., Serrano, E. O., Sanchez-Arguelles, D., Luna, A., Schloerb, F. P., Narayanan, G., Yun, M. S., Sahai, R., Zijlstra, A. A., Chavez-Dagostino, M., Montaña, A., Hughes, D. H., Rodríguez, M.
Extremely high velocity emission likely related to jets is known to occur in some proto-Planetary Nebulae. However, the molecular complexity of this kinematic component is largely unknown. We observed the known extreme outflow from the proto-Planetar
Externí odkaz:
http://arxiv.org/abs/1701.01179
Autor:
Gómez-Ruiz, A. I., Guzman-Ramirez, L., Serrano, E. O., Sánchez-Argüelles, D., Luna, A., Schloerb, F. P., Narayanan, G., Yun, M. S., Sahai, R., Zijlstra, A. A., Chavez-Dagostino, M., Montaña, A., Hughes, D. H., Rodriguez, M.
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters; 2017, Vol. 467 Issue 1, pL61-L65, 5p
