The ALPINE–ALMA [C II] survey: size of individual star-forming galaxies at z= 4–6 and their extended halo structure
S Fujimoto, JD Silverman, M Bethermin… - The Astrophysical …, 2020 - iopscience.iop.org
The Astrophysical Journal, 2020•iopscience.iop.org
We present the physical extent of [C ii] 158 μm line-emitting gas from 46 star-forming
galaxies at z= 4–6 from the ALMA Large Program to INvestigate C ii at Early Times
(ALPINE). Using exponential profile fits, we measure the effective radius of the [C ii] line (${r}
_ {{\rm {e}},[{\rm {C}}{\rm\small {II}}]} $
galaxies at z= 4–6 from the ALMA Large Program to INvestigate C ii at Early Times
(ALPINE). Using exponential profile fits, we measure the effective radius of the [C ii] line (${r}
_ {{\rm {e}},[{\rm {C}}{\rm\small {II}}]} $
Abstract
We present the physical extent of [C ii] 158 μm line-emitting gas from 46 star-forming galaxies at z= 4–6 from the ALMA Large Program to INvestigate C ii at Early Times (ALPINE). Using exponential profile fits, we measure the effective radius of the [C ii] line (${r} _ {{\rm {e}},[{\rm {C}}{\rm\small {II}}]} $
iopscience.iop.org
以上显示的是最相近的搜索结果。 查看全部搜索结果