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9篇 您的检索式：作者名="Strohmayer"

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		题名	作者	年代	出处	被引量
	1	Discovery of a 450 Hz quasi-periodic oscillation from the microquasar GRO J1655-40 with the Rossi X-ray timing explorer显示文摘	Strohmayer T E	2001	ApJ2001，552，：	1
	2	Discovery of a second high-frequency quasi-periodic oscillation from the microquasar GRS 1915+105显示文摘	Strohmayer T E	2001	ApJ2001，554，：	1
	3	Photoassisted dissolution of colloidal manganese dioxide in the presence of phenol显示文摘	Horvá th O Strohmayer K	1998	Journal of Photobiology A: Chemistry1998，116，：	1
	4	An X-Ray pulsar with a super strong magnetic field in the soft gamma-ray repeater SGR1806-20显示文摘	Kouveliotou C Dieters S Strohmayer T		0，，：	1
	5	Discovery of a 450HZ quasi-periodic oscillation from the microquasar GRO J1655 -40 with the rossi X - ray timing explorer显示文摘	Strohmayer T E	2001	Astrophys J2001，552，：	1
	6	Quality issues in the selection of chromite sand for steel foundry use 显示文摘	Scott W D Thomas E M Strohmayer L L	2003	AFS Transactions2003，99，4：	1
	7	Photoredox chemistry of mercury ions in aqueous ethanol solutions显示文摘	Horvá th O Strohmayer K	1999	Joural of Photochemistry A Chemistry1999，128，：	1
	8	Effects of a lecithin and catalase containing semen extender and a second dilution with different enhancing buffers on the quality of cold- stored canine spermatozoa 显示文摘	Kmenta I Strohmayer C Miiller-Schl6 sser F et ol	2011	Theriogenology2011，75，6：	1
	9	Dense matter with eXTP显示文摘In this White Paper we present the potential of the Enhanced X-ray Timing and Polarimetry(eXTP) mission for determining the nature of dense matter; neutron star cores host an extreme density regime which cannot be replicated in a terrestrial laboratory. The tightest statistical constraints on the dense matter equation of state will come from pulse profile modelling of accretion-powered pulsars, burst oscillation sources, and rotation-powered pulsars. Additional constraints will derive from spin measurements, burst spectra, and properties of the accretion flows in the vicinity of the neutron star. Under development by an international Consortium led by the Institute of High Energy Physics of the Chinese Academy of Sciences, the eXTP mission is expected to be launched in the mid 2020 s.	Anna L.Watts WenFei Yu Juri Poutanen Shu Zhang Sudip Bhattacharyya Slavko Bogdanov Long Ji Alessandro Patruno Thomas E.Riley Pavel Bakala Altan Baykal Federico Bernardini Ignazio Bombaci Edward Brown Yuri Cavecchi Deepto Chakrabarty Jér?me Chenevez Nathalie Degenaar Melania Del Santo Tiziana Di Salvo Victor Doroshenko Maurizio Falanga Robert D.Ferdman Marco Feroci Angelo F.Gambino MingYu Ge Svenja K.Greif Sebastien Guillot Can Gungor Dieter H.Hartmann Kai Hebeler Alexander Heger Jeroen Homan Rosario Iaria Jean in 't Zand Oleg Kargaltsev Aleksi KurkelaTheoretical Physics Department CERN XiaoYu Lai Ang Li XiangDong Li ZhaoSheng Li Manuel Linares FangJun Lu Simin Mahmoodifar Mariano Méndez M.Coleman Miller Sharon Morsink Joonas N?ttil? Andrea Possenti Chanda Prescod-Weinstein JinLu Qu Alessandro Riggio Tuomo Salmi Andrea Sanna Andrea Santangelo Hendrik Schatz Achim Schwenk LiMing Song Eva?rámková Benjamin Stappers Holger Stiele Tod Strohmayer Ingo Tews Laura Tolos Gabriel T?r?k David Tsang Martin Urbanec Andrea Vacchi RenXin Xu YuPeng Xu Silvia Zane GuoBao Zhang ShuangNan Zhang WenDa Zhang ShiJie Zheng Xia Zhou	2019	Science China(Physics,Mechanics & Astronomy)2019，62，2：	0

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