Showing 61 - 80 results of 655 for search 'M.', tempo de consulta: 0.11s Limitar resultados
  1. 61
    por ITZIAR ARETXAGA MENDEZ, David Hughes
    Publicado 2009
    ... the Astronomical Thermal Emission Camera (AzTEC). Comparing with existing 850 μm Submillimetre Common-User...
    Ligazón do recurso
    info:eu-repo/semantics/article
  2. 62
    por OLGA MERCEDES VEGA CASANOVA
    Publicado 2010
    ...We make use of Spitzer imaging between 4 and 16 μm and near-infrared data at 2.2 μm to investigate...
    Ligazón do recurso
    info:eu-repo/semantics/article
  3. 63
    por David Hughes
    Publicado 2008
    ...We present high-resolution interferometric imaging of LH 850.02, the brightest 850- and 1200-μm...
    Ligazón do recurso
    info:eu-repo/semantics/article
  4. 64
    por Tovmassian Hrant, Monica Rodriguez
    Publicado 2008
    ...We show that the stellar photored magnitude, m₁₀, of the 10th by brightness galaxy in an Abell...
    Ligazón do recurso
    info:eu-repo/semantics/article
  5. 65
    por JUAN NOE SUAREZ PEREA
    Publicado 2010
    ... with star formation is due to supernovae behaving as cosmic-ray accelerators. To model this emission from M...
    Ligazón do recurso
    info:eu-repo/semantics/masterThesis
  6. 66
    por Itziar Aretxaga, David Hughes
    Publicado 2012
    ... and Infrared Array Camera, and Large APEX Bolometer Camera 870 μm data. Five of the sources (10 per cent) have...
    Ligazón do recurso
    info:eu-repo/semantics/article
  7. 67
    por Itziar Aretxaga, David Hughes
    Publicado 2012
    ... and Infrared Array Camera, and Large APEX Bolometer Camera 870 μm data. Five of the sources (10 per cent) have...
    Ligazón do recurso
    info:eu-repo/semantics/article
  8. 68
    por Gabriel Mellado Villaseñor
    Publicado 2018
    ... utilizados para generar un campo Bessel vectorial (VBB, vector Bessel beam) de orden m. Este campo se...
    Ligazón do recurso
    info:eu-repo/semantics/doctoralThesis
  9. 69
    por JESUS LEONARDO LOPEZ HERNANDEZ
    Publicado 2013
    ... on spiral galaxies M33 and M101. For M33 the central zone was observed together with the external region IC...
    Ligazón do recurso
    info:eu-repo/semantics/doctoralThesis
  10. 70
    ... index of the liquid is higher than that of the ferrule, a liquid MMF with a diameter of 125 μm is formed...
    Ligazón do recurso
    info:eu-repo/semantics/article
  11. 71
    ..., yield upper limits to the dynamical masses for the individual star clusters between 1.8 and 7.1 × 10⁶M...
    Ligazón do recurso
    info:eu-repo/semantics/article
  12. 72
    ..., yield upper limits to the dynamical masses for the individual star clusters between 1.8 and 7.1 × 10⁶M...
    Ligazón do recurso
    info:eu-repo/semantics/article
  13. 73
    por LUIS ABRAHAM SANCHEZ GASPARIANO
    Publicado 2011
    ... in CadenceVirtuoso v5.0.0. of the complete power amplification stage with the UMC 0.18μm Mixed Mode and RF CMOS...
    Ligazón do recurso
    info:eu-repo/semantics/doctoralThesis
  14. 74
    ... circuitos integrados CMOS pozo N Austria Micro Systems (AMS) 0.35 μm y Berkeley 0.13 μm. En base a...
    Ligazón do recurso
    info:eu-repo/semantics/article
  15. 75
    por Maxim Kuznetsov
    Publicado 2019
    ...M dwarf stars are the dominant stellar component of the Galaxy, and therefore they contain...
    Ligazón do recurso
    info:eu-repo/semantics/doctoralThesis
  16. 76
    por Carlos del Burgo Díaz
    Publicado 2013
    ... Herschel/PACS to observe a sample of nearby FGK stars. Data at 100 and 160 μm were obtained, complemented...
    Ligazón do recurso
    info:eu-repo/semantics/article
  17. 77
    por David Hughes
    Publicado 2011
    ... with the AzTEC camera mounted on the Atacama Submillimeter Telescope Experiment (ASTE) 10 m telescope in Chile...
    Ligazón do recurso
    info:eu-repo/semantics/article
  18. 78
    por David Hughes
    Publicado 2010
    ... field from 100 to 500 μm using both PACS and SPIRE. We fit isothermal modified black bodies...
    Ligazón do recurso
    info:eu-repo/semantics/article
  19. 79
    ... ejected by young (t < 20 Myr) and massive (M = 10⁶Mꙩ) coeval stellar cluster with a Salpeter initial mass...
    Ligazón do recurso
    info:eu-repo/semantics/article
  20. 80
    ..., named M3gl. This algorithm contains three components: a new feature representation containing clockwise...
    Ligazón do recurso
    info:eu-repo/semantics/article