glacial
发表于 2025-3-23 13:13:43
Can the Tully-Fisher Relation Be the Result of Initial Conditions?f greater than allowed by observations. Unless halos of spiral galaxies formed at high redshift (. ≳ 1) and did not later accrete any significant amount of mass, the TullyFisher relation is not likely to be the direct result of cosmological initial conditions but rather a consequence of a subsequent feedback process.
舞蹈编排
发表于 2025-3-23 15:32:09
Dark Halo Scaling from Galaxy-Galaxy Lensingnd the upcoming wide-field cameras, super-seeing imaging instruments, and the 8-m class telescopes will provide a great opportunity for the study of the mass distribution of isolated and cluster galaxies.
新陈代谢
发表于 2025-3-23 21:01:59
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公社
发表于 2025-3-24 00:10:07
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MERIT
发表于 2025-3-24 03:32:48
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NOVA
发表于 2025-3-24 06:49:46
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reflection
发表于 2025-3-24 11:27:34
On the Phenomenology of Disk Galaxiesn-linearly with mass. These evidences provide observational constraints to models of disk-galaxy evolution. They find a natural interpretation if it is assumed that the time scale . of protogalaxy collapse is governed primarily by the system initial mass as ...
无价值
发表于 2025-3-24 17:47:29
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neutral-posture
发表于 2025-3-24 20:04:33
Michael Prieler,Florian KohlbacherIn this brief contribution, I will outline hopes of understanding the origin of galaxy scaling relations using numerical simulations as a tool to gain understanding. The case of the Tully-Fisher relation for disk galaxies is used as a working example to illustrate the modest achievements to date and the difficult tasks ahead.
affect
发表于 2025-3-24 23:17:48
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