MIR
发表于 2025-3-25 03:50:50
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aspersion
发表于 2025-3-25 11:17:33
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Coordinate
发表于 2025-3-25 15:39:21
n stars are in that case not metal-rich as previously thought, but they have a metallicity comparable to the LMC, with an age between 0.1–1 Gyr. A significant fraction of the carbon stars still have luminosities fainter than the lower LMC limit of. A similar trend is present among carbon stars found
NIL
发表于 2025-3-25 19:52:46
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erythema
发表于 2025-3-25 23:54:57
Byung Chan Eu are close to those of real spiral and elliptical galaxies. Furthermore, correlations similar to the Tully-Fisher, Faber-Jackson and luminosity-metallicity relations arise quite naturally. A quantitative explanation of the fundamental plane of elliptical galaxies appears within reach.
acrimony
发表于 2025-3-26 02:42:45
n of the medium in which stars are formed, may constitute a break-through of the difficulties in question. Models of elliptical galaxies incorporating the new IMF (varying with time and position inside a galaxy) are presented and discussed at some extent.
Kaleidoscope
发表于 2025-3-26 08:06:27
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oncologist
发表于 2025-3-26 09:31:42
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最高峰
发表于 2025-3-26 13:42:57
Byung Chan Euttheoriginofthebook,IwasaskedbySpringer-Verlagtoexpandtheset of lecture notes that I prepared in 1988 for the First Astrophysics School organised by the European Astrophysics Doctoral Network into a full-length978-3-662-49579-7978-3-540-73478-9Series ISSN 0941-7834 Series E-ISSN 2196-9698
locus-ceruleus
发表于 2025-3-26 18:35:49
ttheoriginofthebook,IwasaskedbySpringer-Verlagtoexpandtheset of lecture notes that I prepared in 1988 for the First Astrophysics School organised by the European Astrophysics Doctoral Network into a full-length978-3-662-49579-7978-3-540-73478-9Series ISSN 0941-7834 Series E-ISSN 2196-9698