EPT
发表于 2025-3-25 04:25:43
http://reply.papertrans.cn/71/7004/700370/700370_21.png
自传
发表于 2025-3-25 07:49:41
Mariko Kimurahistory. If by now we are fairly confident most of these events occurred the way we imagine they occurred, we owe it to a rich suite of cosmological observations, whose precision is ever-increasing. On the other hand, there remain several open questions which near-future cosmological observations mi
察觉
发表于 2025-3-25 13:22:18
http://reply.papertrans.cn/71/7004/700370/700370_23.png
Manifest
发表于 2025-3-25 19:47:56
General Introduction, aim of this dissertation. Dwarf novae are one subclass of cataclysmic variables composed of a white dwarf and a low-mass star. An accretion disk is formed around the white dwarf by the transferred gas from the low-mass star. The most characteristic observational feature of dwarf novae is intermitte
arrogant
发表于 2025-3-25 23:16:29
http://reply.papertrans.cn/71/7004/700370/700370_25.png
调情
发表于 2025-3-26 03:12:55
http://reply.papertrans.cn/71/7004/700370/700370_26.png
Amorous
发表于 2025-3-26 04:48:57
http://reply.papertrans.cn/71/7004/700370/700370_27.png
STAT
发表于 2025-3-26 11:50:24
http://reply.papertrans.cn/71/7004/700370/700370_28.png
BRUNT
发表于 2025-3-26 12:55:58
http://reply.papertrans.cn/71/7004/700370/700370_29.png
运动吧
发表于 2025-3-26 18:11:25
Conclusions, posed in Chap. 1. The conclusion is that the disk-instability model has potential for explaining all kinds of outbursts in dwarf novae if new aspects are taken into account, since this research succeeded to present physically feasible explanations to at least four kinds of newly discovered light va