Identifying dynamically young galaxy groups via wide-angle tail galaxies: a 
case study in the COSMOS field at z = 0.53

Oklopčić, A.; Smolčić, V.; Giodini, S.; Zamorani, G.; Bîrzan, L.; Schinnerer, E.; Carilli, C. L.; Finoguenov, A.; Lilly, S.; Koekemoer, A.; Scoville, N. Z.

doi:10.1088/0004-637X/713/1/484

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Identifying dynamically young galaxy groups via wide-angle tail galaxies: a case study in the COSMOS field at z = 0.53

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Giodini, S.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons16183

Finoguenov, A.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Oklopčić, A., Smolčić, V., Giodini, S., Zamorani, G., Bîrzan, L., Schinnerer, E., Carilli, C. L., Finoguenov, A., Lilly, S., Koekemoer, A., & Scoville, N. Z. (2010). Identifying dynamically young galaxy groups via wide-angle tail galaxies: a case study in the COSMOS field at z = 0.53. The Astrophysical Journal, 713(1), 484-490. doi:10.1088/0004-637X/713/1/484.

引用: https://hdl.handle.net/11858/00-001M-0000-0012-BDC4-4

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