Arrhythmia 发表于 2025-3-30 08:56:03
http://reply.papertrans.cn/31/3029/302865/302865_51.png爱花花儿愤怒 发表于 2025-3-30 14:36:18
http://reply.papertrans.cn/31/3029/302865/302865_52.pngExploit 发表于 2025-3-30 18:39:19
http://reply.papertrans.cn/31/3029/302865/302865_53.pngensemble 发表于 2025-3-30 23:14:40
http://reply.papertrans.cn/31/3029/302865/302865_54.pngRUPT 发表于 2025-3-31 04:22:51
Giulia Massini,Stefano Terzi,Massimo Buscemar. from a curve of growth analysis of the envelope ultraviolet Fell-lines of α Cyg. Radio observations are desirable to make a decision about these discrepant results. Therefore we observed α Cyg at 15 GHz with the 100 m telescope of the MPIfR at Effelsberg. The observations are discussed together with recent VLA data of Abbott et al. (1980).CT-angiography 发表于 2025-3-31 08:37:17
Using Data Mining for CRM Evaluation,ral and singly-ionized metallic lines of very low excitation potential; and 3) asymmetric absorption lines, including H., Hβ, FeI lines of intermediate excitation potential and the infrared triplet of Ca+, which appear to be formed in a relatively warm layer, probably an extended chromosphere.Abominate 发表于 2025-3-31 11:48:30
Book 1981al Physics, Miramare, Trieste (Italy), under the auspices of the IAU Executive Co~ mittee and the Italian National Council of Research. The planning of this conference began two years ago du ring the IAU Symposium No. 83 "Mass loss and evolution of 0 type stars" (Qualicum Beach, Victoria, Canada) w隐士 发表于 2025-3-31 14:38:36
http://reply.papertrans.cn/31/3029/302865/302865_58.pngOrgasm 发表于 2025-3-31 20:00:34
http://reply.papertrans.cn/31/3029/302865/302865_59.png神圣在玷污 发表于 2025-4-1 00:57:08
http://reply.papertrans.cn/31/3029/302865/302865_60.png