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5篇 您的检索式：作者名="A. M. Angulo"

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		题名	作者	年代	出处	被引量
	1	The natural history of nonalcoholic fatty liver disease with advanced fibrosis or cirrhosis: An international collaborative study显示文摘	Neeraj Bhala Paul Angulo David van der Poorten Eric Lee Jason M. Hui Giorgio Saracco Leon A. Adams Phunchai Charatcharoenwitthaya Joanne H. Topping Elisabetta Bugianesi Christopher P. Day Jacob George	2011	Hepatology2011，，4：	2
	2	Leptin, insulin resistance, and liver fibrosis in human nonalcoholic fatty liver disease显示文摘	Paul Angulo Laura M. Alba Lydia M. Petrovic Leon A. Adams Keith D. Lindor Michael D. Jensen	2004	Journal of Hepatology2004，，6：	1
	3	Nosocomial Kikuchi’s Disease – A Search for Herpesvirus Sequences in Lymph Node Tissues Using PCR显示文摘	C. Martinez-Vazquez C. Potel M. Angulo J. Gonzalez-Carreró M. Alvarez A. Tenorio D. Cid I. Oliveira	2001	Infection2001，，3：	1
	4	Genetic variations in host IL 28 B links to the detection of peripheral blood mononuclear cells–associated hepatitis C virus RNA in chronically infected patients显示文摘	J. Angulo K. Pino C. Pavez F. Biel P. Labbé J. F. Miquel A. Soza M. López‐Lastra	2013	J Viral Hepat2013，，：	1
	5	Conceptual design of an experiment to study dust destruction by astrophysical shock waves显示文摘A novel laboratory experimental design is described that will investigate the processing of dust grains in astrophysical shocks. Dust is a ubiquitous ingredient in the interstellar medium(ISM) of galaxies; however, its evolutionary cycle is still poorly understood. Especially shrouded in mystery is the efficiency of grain destruction by astrophysical shocks generated by expanding supernova remnants. While the evolution of these remnants is fairly well understood, the grain destruction efficiency in these shocks is largely unknown. The experiments described herein will fill this knowledge gap by studying the dust destruction efficiencies for shock velocities in the range ~10–30 km/s(μm/ns), at which most of the grain destruction and processing in the ISM takes place. The experiments focus on the study of grain–grain collisions by accelerating small(~1 μm) dust particles into a large(~5–10 μm diameter) population; this simulates the astrophysical system well in that the more numerous, small grains impact and collide with the large population. Facilities that combine the versatility of high-power optical lasers with the diagnostic capabilities of X-ray free-electron lasers, e.g., the Matter in Extreme Conditions instrument at the SLAC National Accelerator Laboratory, provide an ideal laboratory environment to create and diagnose dust destruction by astrophysically relevant shocks at the micron scale.	M. J.-E. Manuel T. Temim E. Dwek A. M. Angulo E X. Belancourt R. E Drake C. C. Kuranz M. J. MacDonald B. A. Remington	2018	High Power Laser Science and Engineering2018，6，3：	0

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