Resolving the ISM at the Peak of Cosmic Star Formation with ALMA: The 
Distribution of CO and Dust Continuum in z {̑ilde} 2.5 Submillimeter Galaxies

Calistro Rivera, G.; Hodge, J.A.; Smail, I.; Swinbank, A.M.; Weiss, A.; Wardlow, J.L.; Walter, F.; Rybak, M.; Chen, C.-C.; Brandt, W.N.; Coppin, K.; da Cunha, E.; Dannerbauer, H.; Greve, T.R.; Karim, A.; Knudsen, K.K.; Schinnerer, E.; Simpson, J.M.; Venemans, B.; van der Werf, P.

doi:10.3847/1538-4357/aacffa

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Resolving the ISM at the Peak of Cosmic Star Formation with ALMA: The Distribution of CO and Dust Continuum in z {̑ilde} 2.5 Submillimeter Galaxies

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Weiss, A.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Calistro Rivera, G., Hodge, J., Smail, I., Swinbank, A., Weiss, A., Wardlow, J., Walter, F., Rybak, M., Chen, C.-C., Brandt, W., Coppin, K., da Cunha, E., Dannerbauer, H., Greve, T., Karim, A., Knudsen, K., Schinnerer, E., Simpson, J., Venemans, B., & van der Werf, P. (2018). Resolving the ISM at the Peak of Cosmic Star Formation with ALMA: The Distribution of CO and Dust Continuum in z {̑ilde} 2.5 Submillimeter Galaxies. Astrophysical Journal, 863:, pp. 56. doi:10.3847/1538-4357/aacffa.

引用: https://hdl.handle.net/21.11116/0000-0004-3CD6-8

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