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541di 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...”
Pubblicazione 2011
Testo
info:eu-repo/semantics/article -
542
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543
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544di OLGA MERCEDES VEGA CASANOVA“... an AGN which accounts for more than 10% of the infrared luminosity from 8 to 1000 μm, whereas all have...”
Pubblicazione 2008
Testo
info:eu-repo/semantics/article -
545di 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...”
Pubblicazione 2010
Testo
info:eu-repo/semantics/article -
546
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547
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548di Manolis Plionis“...¹³h⁻¹Mꙩ. The Xray AGN bias and the corresponding dark-matter host halo mass, are significantly higher...”
Pubblicazione 2012
Testo
info:eu-repo/semantics/article -
549
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550
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551
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552
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553
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554
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555
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556di Sarai Vázquez y Parraguirre“... y concentración de oxigeno permitió reducir la resistencia de hoja del orden de Rs ~ MΩ/□ a Rs = 27...”
Pubblicazione 2016
Testo
info:eu-repo/semantics/masterThesis -
557
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558
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559di MODESTO GUADALUPE MEDINA MELENDREZTesto
Pubblicazione 2010
info:eu-repo/semantics/doctoralThesis -
560di CHRISTOPHER AÑORVE SOLANO“... Clusters, using R-band wide field CCD images obtained with the Kitt Peak National Observatory (KPNO) 0:9 m...”
Pubblicazione 2012
Testo
info:eu-repo/semantics/doctoralThesis