Clumpy galaxies in CANDELS. II. Physical properties of UV-bright clumps at 0.5 ≤ z < 3

Clumpy galaxies in CANDELS. II. Physical properties of UV-bright clumps at 0.5 ≤ z < 3

Studying giant star-forming clumps in distant galaxies is important to understand galaxy formation and evolution. At present, however, observers and theorists have not reached a consensus on whether the observed "clumps" in distant galaxies are the same phenomenon that is seen in simulatio...

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Bibliographic Details
Main Authors: Guo, Yicheng, Rafelski, Marc, Bell, Eric F., Conselice, Christopher J., Dekel, Avishai, Faber, S. M., Giavalisco, Mauro, Koekemoer, Anton M., Koo, David C., Lu, Yu, Mandelker, Nir, Primack, Joel R., Ceverino, Daniel, de Mello, Duilia F., Ferguson, Henry C., Hathi, Nimish, Kocevski, Dale, Lucas, Ray A., Pérez-González, Pablo G., Ravindranath, Swara, Soto, Emmaris, Straughn, Amber, Wang, Weichen
Format: Article
Published: American Astronomical Society 2018
Subjects:
galaxies: evolution ; galaxies: formation ; galaxies: starburst ; galaxies: star formation ; galaxies: structure ; ultraviolet: galaxies
Online Access:https://eprints.nottingham.ac.uk/49664/

Internet

https://eprints.nottingham.ac.uk/49664/

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