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pro vyhledávání: '"Lee, Cristoph T."'
Autor:
Lin, Lin, Faber, S. M., Koo, David C., Salim, Samir, Dutton, Aaron A., Fang, Jerome J., Jiang, Fangzhou, Lee, Cristoph T., Rodríguez-Puebla, Aldo, van der Wel, A., Guo, Yicheng, Barro, Guillermo, Primack, Joel R., Dekel, Avishai, Chen, Zhu, Luo, Yifei, Pandya, Viraj, Somerville, Rachel S., Ferguson, Henry C., Kassin, Susan, Koekemoer, Anton M., Grogin, Norman A., Galametz, Audrey, Santini, P., Nayyeri, Hooshang, Stefanon, Mauro, Dahlen, Tomas, Mobasher, Bahram, Hao, Lei
This paper is one in a series that explores the importance of radius as a second parameter in galaxy evolution. The topic investigated here is the relationship between star formation rate (SFR) and galaxy radius ($R_{\rm e}$) for main-sequence star-f
Externí odkaz:
http://arxiv.org/abs/1910.10947