enormous 发表于 2025-3-27 00:09:38
http://reply.papertrans.cn/25/2420/241996/241996_31.pngSedative 发表于 2025-3-27 03:33:23
http://reply.papertrans.cn/25/2420/241996/241996_32.png烧烤 发表于 2025-3-27 07:42:02
Michele Trimarchi,Paolo Manzelli89 Herculis (F2Ia/Ib) is a pulsating binary (Smolinski et al. 1980; Waters et al. 1993) fulfilling the criteria for low-mass post-AGB stars.地名词典 发表于 2025-3-27 12:30:19
https://doi.org/10.1007/978-3-030-67956-9We observed the 22 GHz water maser emission in VX UMa (M8e, M=388.) and V778 Cyg (C5,5J, SRb=300.) from 1987-1992. The spectra of both stars show three distinct components. All three components vary periodically in intensity. We interpret these features as being produced by a rotating circumstellar disk河潭 发表于 2025-3-27 14:50:40
http://reply.papertrans.cn/25/2420/241996/241996_35.png隼鹰 发表于 2025-3-27 19:41:54
http://reply.papertrans.cn/25/2420/241996/241996_36.pngConsole 发表于 2025-3-28 01:40:36
http://reply.papertrans.cn/25/2420/241996/241996_37.pngMatrimony 发表于 2025-3-28 04:26:02
Variable Water Maser Emission from Circumstellar DisksWe observed the 22 GHz water maser emission in VX UMa (M8e, M=388.) and V778 Cyg (C5,5J, SRb=300.) from 1987-1992. The spectra of both stars show three distinct components. All three components vary periodically in intensity. We interpret these features as being produced by a rotating circumstellar disk愤愤不平 发表于 2025-3-28 07:37:07
http://reply.papertrans.cn/25/2420/241996/241996_39.pngFLOUR 发表于 2025-3-28 13:16:49
978-3-662-11392-9Springer-Verlag Berlin Heidelberg 1998