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541по Elena Kirilovsky Terlevich“... or to an expanding bubble or shell of the ionized gas approaching us. A dynamical mass of 2.5×10¹°Mꙩ is derived from...”
Опубликовано 2011
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542по CARLOS MANUEL HERNANDEZ MEJIAПолный текст
Опубликовано 2015
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544по OLGA MERCEDES VEGA CASANOVA“... an AGN which accounts for more than 10% of the infrared luminosity from 8 to 1000 μm, whereas all have...”
Опубликовано 2008
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545по JESUS EZEQUIEL MOLINAR SOLIS, VICTOR HUGO PONCE PONCE, RODOLFO ZOLA GARCIA LOZANO, ALEJANDRO DIAZ SANCHEZ, JOSE MIGUEL ROCHA PEREZ“... with 1.2 μm design rules, were compared. the extracted parameters can be incorporated into floating-gate ps...”
Опубликовано 2010
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548по Manolis Plionis“...¹³h⁻¹Mꙩ. The Xray AGN bias and the corresponding dark-matter host halo mass, are significantly higher...”
Опубликовано 2012
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553по MARIA ALEJANDRA MENENDEZ ORTIZПолный текст
Опубликовано 2012
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556по Sarai Vázquez y Parraguirre“... y concentración de oxigeno permitió reducir la resistencia de hoja del orden de Rs ~ MΩ/□ a Rs = 27...”
Опубликовано 2016
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557по ROGELIO MANUEL HIGUERA GONZALEZПолный текст
Опубликовано 2017
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558по MIGUEL AURELIO DUARTE VILLASEÑORПолный текст
Опубликовано 2010
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559по MODESTO GUADALUPE MEDINA MELENDREZПолный текст
Опубликовано 2010
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560по CHRISTOPHER AÑORVE SOLANO“... Clusters, using R-band wide field CCD images obtained with the Kitt Peak National Observatory (KPNO) 0:9 m...”
Опубликовано 2012
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info:eu-repo/semantics/doctoralThesis