Background X-Ray Emission from Hot Gas in CDM and CDM+ Lambda Universes: Spectral Signatures
نویسندگان
چکیده
منابع مشابه
Background X-ray Emission from Hot Gas in Cdm and Cdm+λ Universes: Spectral Signatures
We present a new treatment of two popular models for the growth of structure, examining the X-ray emission from hot gas with allowance for spectral line emission from various atomic species, primarily “metals”. The X-ray emission from the bright cluster sources is not significantly changed from prior work and, as noted earlier, shows the CDM+Λ model (LCDM) to be consistent but the standard, COB...
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We present a new treatment of two popular models for the growth of structure, examining the X-ray emission from hot gas with allowance for spectral line emission from various atomic species, primarily \metals". The X-ray emission from the bright cluster sources is not signi cantly changed from prior work and, as noted earlier, shows the CDM+ model (LCDM) to be consistent but the standard, COBE ...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 1995
ISSN: 0004-637X,1538-4357
DOI: 10.1086/176232