hauteur 发表于 2025-3-30 09:45:01

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描述 发表于 2025-3-30 14:34:34

UV Excess and AGB Evolution in Elliptical-Galaxy Stellar Populations, contributors to galaxy ultraviolet luminosity excess. While a blue HB morphology seems a natural characteristic of metal-poor stellar populations, its appearance in metal-rich systems, often coupled with a poorer rate of planetary nebulae per unit galaxy luminosity, might be calling for an intimate

ear-canal 发表于 2025-3-30 17:21:33

Binary Stars as the Source of the Far-UV Excess in Elliptical Galaxies,at this UV excess is caused by an old population of hot helium-burning stars without large hydrogen-rich envelopes rather than young stars, their origin has remained a mystery. Here we show that these stars most likely lost their envelopes because of binary interactions, similar to the hot subdwarf

Mystic 发表于 2025-3-31 00:24:35

,Stellar Populations in Field Early–Type Galaxies,tudy from ultraviolet (UV) to infrared (IR) of a sample 65 nearby ETGs. We derived Lick line-strength indices at different galacto-centric distances from the optical spectra (3700-7000 Å), and extracted ages, metallicites and element abundance ratios for the galaxies by comparison of the indices wit

resuscitation 发表于 2025-3-31 03:35:42

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钱财 发表于 2025-3-31 07:34:49

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大喘气 发表于 2025-3-31 10:51:13

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无王时期, 发表于 2025-3-31 16:23:19

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LINE 发表于 2025-3-31 20:09:10

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correspondent 发表于 2025-3-31 21:49:27

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查看完整版本: Titlebook: New Quests in Stellar Astrophysics II; Ultraviolet Properti Miguel‘Chavez Dagostino Conference proceedings 2009 The Editor(s) (if applicabl