Showing 61 - 80 results of 655 for search 'M.', query time: 0.43s Refine Results
  1. 61
    ... the Astronomical Thermal Emission Camera (AzTEC). Comparing with existing 850 μm Submillimetre Common-User...
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  2. 62
    by OLGA MERCEDES VEGA CASANOVA
    Published 2010
    ...We make use of Spitzer imaging between 4 and 16 μm and near-infrared data at 2.2 μm to investigate...
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  3. 63
    by David Hughes
    Published 2008
    ...We present high-resolution interferometric imaging of LH 850.02, the brightest 850- and 1200-μm...
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  4. 64
    by Tovmassian Hrant, Monica Rodriguez
    Published 2008
    ...We show that the stellar photored magnitude, m₁₀, of the 10th by brightness galaxy in an Abell...
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  5. 65
    by JUAN NOE SUAREZ PEREA
    Published 2010
    ... with star formation is due to supernovae behaving as cosmic-ray accelerators. To model this emission from M...
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    info:eu-repo/semantics/masterThesis
  6. 66
    by Itziar Aretxaga, David Hughes
    Published 2012
    ... and Infrared Array Camera, and Large APEX Bolometer Camera 870 μm data. Five of the sources (10 per cent) have...
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  7. 67
    by Itziar Aretxaga, David Hughes
    Published 2012
    ... and Infrared Array Camera, and Large APEX Bolometer Camera 870 μm data. Five of the sources (10 per cent) have...
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  8. 68
    by Gabriel Mellado Villaseñor
    Published 2018
    ... utilizados para generar un campo Bessel vectorial (VBB, vector Bessel beam) de orden m. Este campo se...
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    info:eu-repo/semantics/doctoralThesis
  9. 69
    by JESUS LEONARDO LOPEZ HERNANDEZ
    Published 2013
    ... on spiral galaxies M33 and M101. For M33 the central zone was observed together with the external region IC...
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    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...
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  11. 71
    ..., yield upper limits to the dynamical masses for the individual star clusters between 1.8 and 7.1 × 10⁶M...
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  12. 72
    ..., yield upper limits to the dynamical masses for the individual star clusters between 1.8 and 7.1 × 10⁶M...
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  13. 73
    ... in CadenceVirtuoso v5.0.0. of the complete power amplification stage with the UMC 0.18μm Mixed Mode and RF CMOS...
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  14. 74
    ... circuitos integrados CMOS pozo N Austria Micro Systems (AMS) 0.35 μm y Berkeley 0.13 μm. En base a...
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  15. 75
    by Maxim Kuznetsov
    Published 2019
    ...M dwarf stars are the dominant stellar component of the Galaxy, and therefore they contain...
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    info:eu-repo/semantics/doctoralThesis
  16. 76
    by Carlos del Burgo Díaz
    Published 2013
    ... Herschel/PACS to observe a sample of nearby FGK stars. Data at 100 and 160 μm were obtained, complemented...
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  17. 77
    by David Hughes
    Published 2011
    ... with the AzTEC camera mounted on the Atacama Submillimeter Telescope Experiment (ASTE) 10 m telescope in Chile...
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  18. 78
    by David Hughes
    Published 2010
    ... field from 100 to 500 μm using both PACS and SPIRE. We fit isothermal modified black bodies...
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  19. 79
    ... ejected by young (t < 20 Myr) and massive (M = 10⁶Mꙩ) coeval stellar cluster with a Salpeter initial mass...
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  20. 80
    ..., named M3gl. This algorithm contains three components: a new feature representation containing clockwise...
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