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The metallicity dependence of the CO → H2 conversion factor in z ≥ 1 star-forming galaxies

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Genzel,  R.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Tacconi,  L. J.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Förster Schreiber,  N. M.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Gracia-Carpio,  J.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Lutz,  D.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Naab,  T.
Cosmology, MPI for Astrophysics, Max Planck Society;

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Saintonge,  A.
Cosmology, MPI for Astrophysics, Max Planck Society;
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Citation

Genzel, R., Tacconi, L. J., Combes, F., Bolatto, A., Neri, R., Sternberg, A., et al. (2012). The metallicity dependence of the CO → H2 conversion factor in z ≥ 1 star-forming galaxies. The Astrophysical Journal, 746(1): 69, pp. 1-11. doi:10.1088/0004-637X/746/1/69.


Cite as: https://hdl.handle.net/11858/00-001M-0000-000E-B1AD-C
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