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Starburst Galaxies at High Redshift
1997The properties of ultraluminous and hyperluminous galaxies are reviewed and it is argued that the majority of the far infrared radiation from these galaxies is powered by starbursts. The evidence that the starburst population is also seen in the sub-mJy radio source-counts is reviewed and a model for the source-counts from radio to X-rays is presented.
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Maximum Correntropy Based Spectral Redshift Estimation for Spectral Redshift Navigation
IEEE Transactions on Instrumentation and Measurement, 2023Guangle Gao, Yongmin Zhong, Zhaohui Gao
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Galaxy Morphology at High Redshift
2014The morphology of galaxies at high redshift ranges from elliptical and spiral to clumpy, including chains, clump clusters, doubles and tadpoles. Clumpy galaxies observed in the Hubble Ultra Deep Field at redshifts z = 1–5 contain star-forming complexes that are hundreds of times more massive than those forming in local galaxies, reflecting the more ...
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1997
Study of molecular gas in distant galaxies during the last twenty years has followed the steady progress in mm wave receiver sensitivity. In 1975, CO was detected in M 82, NGC 253, and several other galaxies with redshifts of a few hundred kms−1 (Rickard et al. 1975; Solomon & de Zafra 1975).
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Study of molecular gas in distant galaxies during the last twenty years has followed the steady progress in mm wave receiver sensitivity. In 1975, CO was detected in M 82, NGC 253, and several other galaxies with redshifts of a few hundred kms−1 (Rickard et al. 1975; Solomon & de Zafra 1975).
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Measuring dynamical masses from gas kinematics in simulated high-redshift galaxies
Monthly Notices of the Royal Astronomical Society, 2020Sarah Wellons +2 more
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On the dust temperatures of high-redshift galaxies
Monthly Notices of the Royal Astronomical Society, 2019Lichen Liang +2 more
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Traversable wormholes in f(R) gravity with constant and variable redshift functions
New Astronomy, 2020Nisha Godani, Gauranga C Samanta
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