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    Gone with the heat

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    0258_Gonewiththeheat.pdf (1.730Mb)
    Date
    2016
    Author
    Zhang, Zhi-Yu
    P. Papadopoulos, Padelis
    R. J. Ivison
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    Abstract
    Images of dust continuum and carbon monoxide (CO) line emission are powerful tools for deducing structural characteristics of galaxies, such as disc sizes, H2 gas velocity fields and enclosed H2 and dynamical masses. We report on a fundamental constraint set by the cosmic microwave background (CMB) on the observed structural and dynamical characteristics of galaxies, as deduced from dust continuum and CO-line imaging at high redshifts
    URI
    https://lib.hpu.edu.vn/handle/123456789/21891
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