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ATOMIUM: The astounding complexity of the near circumstellar environment of the M-type AGB star R Hydrae. I. Morpho-kinematical interpretation of CO and SiO emission

MPS-Authors

Jeste,  Manali
Max Planck Institute for Radio Astronomy, Max Planck Society;

Menten,  Karl
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Homan, W., Pimpanuwat, B., Herpin, F., Danilovich, T., McDonald, I., Wallström, S. H., Richards, A. M., Baudry, A., Sahai, R., Millar, T. J., de Koter, A., Gottlieb, C.-A., Kervella, P., Montargès, M., Van de Sande, M., Decin, L., Zijlstra, A., Etoka, S., Jeste, M., Müller, H. S., Maes, S., Malfait, J., Menten, K., Plane, J., Lee, K., Waters, R., Wong, K. T., Lagadec, E., Gobrecht, D., Yates, J., Price, D., Cannon, E., Bolte, J., De Ceuster, F., Nuth, J., Philip Sindel, J., Kee, D., Gray, M. D., & El Mellah, I. (2021). ATOMIUM: The astounding complexity of the near circumstellar environment of the M-type AGB star R Hydrae. I. Morpho-kinematical interpretation of CO and SiO emission. åp, 651:, pp. A82. doi:10.1051/0004-6361/202140512.


引用: https://hdl.handle.net/21.11116/0000-000A-71EE-B
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