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  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., 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.

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 Creators:
Tyler, K. D., Author
Rieke, G. H., Author
Wilman, D. J.1, Author              
McGee, S. L., Author
Bower, R. G., Author
Bai, L., Author
Mulchaey, J. S., Author
Parker, L. C., Author
Shi, Y., Author
Pierini, D.2, Author              
Affiliations:
1Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society, ou_159895              
2High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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Language(s): eng - English
 Dates: 2011-09-01
 Publication Status: Published in print
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1088/0004-637X/738/1/56
 Degree: -

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Title: The Astrophysical Journal
  Abbreviation : Astrophys. J.
Source Genre: Journal
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Pages: - Volume / Issue: 738 (1) Sequence Number: 56 Start / End Page: 1 - 14 Identifier: ISSN: 0004-637x