ALMA characterizes the dust temperature of z ∼ 5.5 star-forming galaxies
نویسندگان
چکیده
منابع مشابه
The Dust Attenuation of Star-forming Galaxies at z ∼ 3 and Beyond: New Insights from ALMA Observations
We present results on the dust attenuation of galaxies at redshift ∼ 3 − 6 by studying the relationship between the UV spectral slope (βUV) and the infrared excess (IRX; LIR/LUV) using ALMA far-infrared continuum observations. Our study is based on a sample of 67 massive, star-forming galaxies with a median mass of M∗∼ 10 10.7 M⊙ spanning a redshift range z = 2.6−3.7 (median z = 3.2) that were ...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2020
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/staa2545