The nature of star formation at 24 μm in the group environment at 0.3 z 0.55

Tyler, K. D.; Rieke, G. H.; Wilman, D. J.; McGee, S. L.; Bower, R. G.; Bai, L.; Mulchaey, J. S.; Parker, L. C.; Shi, Y.; Pierini, D.

doi:10.1088/0004-637X/738/1/56

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The nature of star formation at 24 μm in the group environment at 0.3 z 0.55

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Wilman, D. J.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Pierini, D.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Tyler, K. D., Rieke, G. H., Wilman, D. J., McGee, S. L., Bower, R. G., Bai, L., et al. (2011). The nature of star formation at 24 μm in the group environment at 0.3 z 0.55. The Astrophysical Journal, 738(1): 56, pp. 1-14. doi:10.1088/0004-637X/738/1/56.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0012-28E0-8

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