ALIBI
发表于 2025-3-26 22:10:54
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hidebound
发表于 2025-3-27 03:29:31
Itamar Francezy Fabian and colleagues at Cambridge as a p- sible explanation of the physical processes obtained in the central regions of clusters. The name refers to the fact that gas cooling in the inner regions is associated with a loss of central pressure, causin978-3-642-09257-2978-3-540-73484-0Series ISSN 1431-2433 Series E-ISSN 1611-6143
COMA
发表于 2025-3-27 05:38:36
Yulia Dubov,Michael Kaminskiy Fabian and colleagues at Cambridge as a p- sible explanation of the physical processes obtained in the central regions of clusters. The name refers to the fact that gas cooling in the inner regions is associated with a loss of central pressure, causin978-3-642-09257-2978-3-540-73484-0Series ISSN 1431-2433 Series E-ISSN 1611-6143
他一致
发表于 2025-3-27 12:49:40
Daniel Lehmanny Fabian and colleagues at Cambridge as a p- sible explanation of the physical processes obtained in the central regions of clusters. The name refers to the fact that gas cooling in the inner regions is associated with a loss of central pressure, causin978-3-642-09257-2978-3-540-73484-0Series ISSN 1431-2433 Series E-ISSN 1611-6143
jagged
发表于 2025-3-27 16:31:33
the gaseous baryons did not cool, collapse, and form stars and galaxies. However, if this gas is allowed to cool unimpeded at the rate predicted from known atomic physics, in the context of a well-established cosmological model, the gaseous matter would form stars and galaxies with a high e?ciency,
Offstage
发表于 2025-3-27 21:01:57
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A保存的
发表于 2025-3-28 00:06:06
Ron Artstein,Sudeep Gandhe,Jillian Gerten,Anton Leuski,David Traumthe gaseous baryons did not cool, collapse, and form stars and galaxies. However, if this gas is allowed to cool unimpeded at the rate predicted from known atomic physics, in the context of a well-established cosmological model, the gaseous matter would form stars and galaxies with a high e?ciency,
Fluctuate
发表于 2025-3-28 03:25:48
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倔强不能
发表于 2025-3-28 08:17:47
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平躺
发表于 2025-3-28 12:12:14
Nachum Dershowitzd to cool unimpeded at the rate predicted from known atomic physics, in the context of a well-established cosmological model, the gaseous matter would form stars and galaxies with a high e?ciency, so that far more than the observed fraction of about 10–15% of the baryonic matter would be found in lu