comely 发表于 2025-3-28 15:21:33
Daniel J. Gough,Pravin Sehgal,David E. Levyrst of all, full-scale frame and point-supported glass façades, incorporating single, double and coated glazing, were tested under pool fire conductions. The results determined the effects of different glass frames, types of glass, and thermal shocks on breakage behavior. Small-scale tests, using th微枝末节 发表于 2025-3-28 21:27:53
http://reply.papertrans.cn/51/5004/500358/500358_42.pngreject 发表于 2025-3-29 00:34:16
http://reply.papertrans.cn/51/5004/500358/500358_43.png单调女 发表于 2025-3-29 04:02:07
http://reply.papertrans.cn/51/5004/500358/500358_44.png补充 发表于 2025-3-29 08:20:44
Harini Nivarthi,Katrin Friedbichler,Richard Moriggl1992. The objective of the workshop was to bring together a select group of theoreticians and experimental biologists to present the latest results in the area of biological pattern formation and to foster interactiqn across dis- plines. The workshop was divided into 5 main areas: (i) limb developme泛滥 发表于 2025-3-29 14:41:29
Haiyan S. Li,Stephanie S. Watowichly because of the lack of a good observational guidance. One major conceptual problem in massive star formation arises from the radiation pressure they exert on the surrounding dust and gas, which could be strong enough to halt further accretion and impose a limit to the mass of a star. Radiation hyorient 发表于 2025-3-29 17:15:01
Eva Maria Putz,Eva Zebedin,Veronika Sexld a hydrodynamic model in order to study dark matter halos of galaxies. The theoretical general idea is to start with the Einstein–Hilbert Lagrangian in which we have added a complex scalar field minimally coupled to the geometry. Then, by making variations of the corresponding action we come up witAbsenteeism 发表于 2025-3-29 22:30:41
Alejandro Villarino,Xiang-Ping Yang,Kiyoshi Hirahara,Yuka Kanno,John J. O’ Shea,Arian Laurencely because of the lack of a good observational guidance. One major conceptual problem in massive star formation arises from the radiation pressure they exert on the surrounding dust and gas, which could be strong enough to halt further accretion and impose a limit to the mass of a star. Radiation hyIndolent 发表于 2025-3-30 00:25:37
Damla Olcaydu,Robert Kralovicsterials. However, it has two undesirable properties, namely: low tensile strength and large brittleness that cause the collapse to occur shortly after the formation of the first crack. To improve these two negative properties and to achieve a partial substitute of conventional reinforcement, an addifidelity 发表于 2025-3-30 06:36:00
Jeffrey W. Schmidt,Kay-Uwe Wagnerterials. However, it has two undesirable properties, namely: low tensile strength and large brittleness that cause the collapse to occur shortly after the formation of the first crack. To improve these two negative properties and to achieve a partial substitute of conventional reinforcement, an addi