Näytetään 61 - 80 yhteensä 655 tuloksesta haulle 'M.', hakuaika: 0,28s Tarkenna hakua
  1. 61
    Tekijä ITZIAR ARETXAGA MENDEZ, David Hughes
    Julkaistu 2009
    ... the Astronomical Thermal Emission Camera (AzTEC). Comparing with existing 850 μm Submillimetre Common-User...
    Hae kokoteksti
    info:eu-repo/semantics/article
  2. 62
    Tekijä OLGA MERCEDES VEGA CASANOVA
    Julkaistu 2010
    ...We make use of Spitzer imaging between 4 and 16 μm and near-infrared data at 2.2 μm to investigate...
    Hae kokoteksti
    info:eu-repo/semantics/article
  3. 63
    Tekijä David Hughes
    Julkaistu 2008
    ...We present high-resolution interferometric imaging of LH 850.02, the brightest 850- and 1200-μm...
    Hae kokoteksti
    info:eu-repo/semantics/article
  4. 64
    Tekijä Tovmassian Hrant, Monica Rodriguez
    Julkaistu 2008
    ...We show that the stellar photored magnitude, m₁₀, of the 10th by brightness galaxy in an Abell...
    Hae kokoteksti
    info:eu-repo/semantics/article
  5. 65
    Tekijä JUAN NOE SUAREZ PEREA
    Julkaistu 2010
    ... with star formation is due to supernovae behaving as cosmic-ray accelerators. To model this emission from M...
    Hae kokoteksti
    info:eu-repo/semantics/masterThesis
  6. 66
    Tekijä Itziar Aretxaga, David Hughes
    Julkaistu 2012
    ... and Infrared Array Camera, and Large APEX Bolometer Camera 870 μm data. Five of the sources (10 per cent) have...
    Hae kokoteksti
    info:eu-repo/semantics/article
  7. 67
    Tekijä Itziar Aretxaga, David Hughes
    Julkaistu 2012
    ... and Infrared Array Camera, and Large APEX Bolometer Camera 870 μm data. Five of the sources (10 per cent) have...
    Hae kokoteksti
    info:eu-repo/semantics/article
  8. 68
    Tekijä Gabriel Mellado Villaseñor
    Julkaistu 2018
    ... utilizados para generar un campo Bessel vectorial (VBB, vector Bessel beam) de orden m. Este campo se...
    Hae kokoteksti
    info:eu-repo/semantics/doctoralThesis
  9. 69
    Tekijä JESUS LEONARDO LOPEZ HERNANDEZ
    Julkaistu 2013
    ... on spiral galaxies M33 and M101. For M33 the central zone was observed together with the external region IC...
    Hae kokoteksti
    info:eu-repo/semantics/doctoralThesis
  10. 70
    Tekijä José Javier Sánchez Mondragón
    Julkaistu 2013
    ... index of the liquid is higher than that of the ferrule, a liquid MMF with a diameter of 125 μm is formed...
    Hae kokoteksti
    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...
    Hae kokoteksti
    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...
    Hae kokoteksti
    info:eu-repo/semantics/article
  13. 73
    Tekijä LUIS ABRAHAM SANCHEZ GASPARIANO
    Julkaistu 2011
    ... in CadenceVirtuoso v5.0.0. of the complete power amplification stage with the UMC 0.18μm Mixed Mode and RF CMOS...
    Hae kokoteksti
    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...
    Hae kokoteksti
    info:eu-repo/semantics/article
  15. 75
    Tekijä Maxim Kuznetsov
    Julkaistu 2019
    ...M dwarf stars are the dominant stellar component of the Galaxy, and therefore they contain...
    Hae kokoteksti
    info:eu-repo/semantics/doctoralThesis
  16. 76
    Tekijä Carlos del Burgo Díaz
    Julkaistu 2013
    ... Herschel/PACS to observe a sample of nearby FGK stars. Data at 100 and 160 μm were obtained, complemented...
    Hae kokoteksti
    info:eu-repo/semantics/article
  17. 77
    Tekijä David Hughes
    Julkaistu 2011
    ... with the AzTEC camera mounted on the Atacama Submillimeter Telescope Experiment (ASTE) 10 m telescope in Chile...
    Hae kokoteksti
    info:eu-repo/semantics/article
  18. 78
    Tekijä David Hughes
    Julkaistu 2010
    ... field from 100 to 500 μm using both PACS and SPIRE. We fit isothermal modified black bodies...
    Hae kokoteksti
    info:eu-repo/semantics/article
  19. 79
    Tekijä ROBERTO GIOVANNI TERLEVICH AFONSO
    Julkaistu 2012
    ... ejected by young (t < 20 Myr) and massive (M = 10⁶Mꙩ) coeval stellar cluster with a Salpeter initial mass...
    Hae kokoteksti
    info:eu-repo/semantics/article
  20. 80
    ..., named M3gl. This algorithm contains three components: a new feature representation containing clockwise...
    Hae kokoteksti
    info:eu-repo/semantics/article