201. The Origins of UV–optical Color Gradients in Star-forming Galaxies at z ∼ 2: Predominant Dust Gradients but Negligible sSFR Gradients
- Author
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Jerome J. Fang, Yicheng Guo, Hassen M. Yesuf, F. S. Liu, Xianzhong Zheng, Shude Mao, Lu Liu, Wei Tong, Sandro Tacchella, Dongfei Jiang, S. M. Faber, Guillermo Barro, Weichen Wang, Xian-Min Meng, David C. Koo, and Meng Jia
- Subjects
Physics ,Stellar mass ,010308 nuclear & particles physics ,Star formation ,Star (game theory) ,FOS: Physical sciences ,Spectral density ,Astronomy and Astrophysics ,Radius ,Astrophysics ,Noon ,Astrophysics - Astrophysics of Galaxies ,01 natural sciences ,Galaxy ,Space and Planetary Science ,Astrophysics of Galaxies (astro-ph.GA) ,0103 physical sciences ,010303 astronomy & astrophysics - Abstract
The rest-frame UV-optical (i.e., $NUV-B$) color is sensitive to both low-level recent star formation (specific star formation rate - sSFR) and dust. In this Letter, we extend our previous work on the origins of $NUV-B$ color gradients in star-forming galaxies (SFGs) at $z\sim1$ to those at $z\sim2$. We use a sample of 1335 large (semi-major axis radius $R_{\rm SMA}>0.''18$) SFGs with extended UV emission out to $2R_{\rm SMA}$ in the mass range $M_{\ast} = 10^{9}-10^{11}M_{\odot}$ at $1.5, Comment: 10 pages, 4 figures, 1 table, accepted for publication in ApJL
- Published
- 2017