hauteur 发表于 2025-3-30 09:45:01
http://reply.papertrans.cn/67/6658/665703/665703_51.png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 intimateear-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 subdwarfMystic 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 witresuscitation 发表于 2025-3-31 03:35:42
http://reply.papertrans.cn/67/6658/665703/665703_55.png钱财 发表于 2025-3-31 07:34:49
http://reply.papertrans.cn/67/6658/665703/665703_56.png大喘气 发表于 2025-3-31 10:51:13
http://reply.papertrans.cn/67/6658/665703/665703_57.png无王时期, 发表于 2025-3-31 16:23:19
http://reply.papertrans.cn/67/6658/665703/665703_58.pngLINE 发表于 2025-3-31 20:09:10
http://reply.papertrans.cn/67/6658/665703/665703_59.pngcorrespondent 发表于 2025-3-31 21:49:27
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