Gone with the heat

Please use this identifier to cite or link to this item: https://lib.hpu.edu.vn/handle/123456789/21891

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DC Field	Value	Language
dc.contributor.author	Zhang, Zhi-Yu	en_US
dc.contributor.author	P. Papadopoulos, Padelis	en_US
dc.contributor.author	R. J. Ivison	en_US
dc.date.accessioned	2016-07-04T03:49:02Z
dc.date.available	2016-07-04T03:49:02Z
dc.date.issued	2016	en_US
dc.identifier.other	HPU4160375	en_US
dc.identifier.uri	https://lib.hpu.edu.vn/handle/123456789/21891	-
dc.description.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	en_US
dc.format.extent	13 p.	en_US
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en_US
dc.subject	Astronomy	en_US
dc.subject	Astrophysics	en_US
dc.subject	Interstellar medium	en_US
dc.subject	Galaxies	en_US
dc.subject	interstellar medium	en_US
dc.subject	Cosmology	en_US
dc.subject	Cosmic background radiation	en_US
dc.subject	Galaxies	en_US
dc.subject	High redshift	en_US
dc.title	Gone with the heat	en_US
dc.type	Article	en_US
dc.size	1.73MB	en_US
dc.department	Education	en_US
Appears in Collections:	Education

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