Chapter 21: Reflection and Refraction
... magician wants you to believe? You probably would not. Maybe the magician hid another vile in the oil prior to the experiment and just picked it out at the right time? But how could the magician hide an unbroken vile in transparent oil through which you can see? In this chapter you will learn how to ...
... magician wants you to believe? You probably would not. Maybe the magician hid another vile in the oil prior to the experiment and just picked it out at the right time? But how could the magician hide an unbroken vile in transparent oil through which you can see? In this chapter you will learn how to ...
Basics of Polarizing Microscopy
... interference color chart. By comparing the interference color of the anisotropy with the interference color chart, the retardation of the anisotropy can be estimated. A vertical line is drawn on the interference color chart to show the relationship between double refraction (n e -n o ) and the thick ...
... interference color chart. By comparing the interference color of the anisotropy with the interference color chart, the retardation of the anisotropy can be estimated. A vertical line is drawn on the interference color chart to show the relationship between double refraction (n e -n o ) and the thick ...
Mapping the Dark Matter
... Determining Star Formation History from Galaxy Spectra • Various indicators ...
... Determining Star Formation History from Galaxy Spectra • Various indicators ...
Present
... The SWIRE Spitzer survey has detected by far the largest set of Sub-Millimeter Galaxies (SMG) But their identification is difficult and requires validation with (sub-)millimeter observations With MAMBO/IRAM we detected at 1.2mm 20 SWIRE z~2 starburst HLIRGs with LFIR~1013Lo They belong to a rather r ...
... The SWIRE Spitzer survey has detected by far the largest set of Sub-Millimeter Galaxies (SMG) But their identification is difficult and requires validation with (sub-)millimeter observations With MAMBO/IRAM we detected at 1.2mm 20 SWIRE z~2 starburst HLIRGs with LFIR~1013Lo They belong to a rather r ...
View/Open - University of Hertfordshire
... distinguish between members of NGC 6822 and foreground stars in the Milky Way and that the analysis tools available could be used to obtain useful velocity results from the spectra. This led to the discovery of a rotating population of intermediate age stars in the halo of NGC 6822, which constitute ...
... distinguish between members of NGC 6822 and foreground stars in the Milky Way and that the analysis tools available could be used to obtain useful velocity results from the spectra. This led to the discovery of a rotating population of intermediate age stars in the halo of NGC 6822, which constitute ...
Galaxy Formation
... • galaxies are receding from us with speed proportional to their distance • expansion is the same for all observers 2. The microwave background radiation ...
... • galaxies are receding from us with speed proportional to their distance • expansion is the same for all observers 2. The microwave background radiation ...
CHAPTER 10 Light as a wave
... ■■ discuss the results of Young’s double-slit experiment as evidence for the wavelike nature of light in terms of the constructive and destructive interference of waves ■■ interpret the pattern produced by light when it passes through a small gap or past an obstacle in terms of the diffraction of w ...
... ■■ discuss the results of Young’s double-slit experiment as evidence for the wavelike nature of light in terms of the constructive and destructive interference of waves ■■ interpret the pattern produced by light when it passes through a small gap or past an obstacle in terms of the diffraction of w ...
Nobuyuki Kawai
... Eiso=4x1052 erg Strong beaming x100 unseen (off beam axis) short GRB! • many more target events for GW! • no regular “GRB”: how to identify? – may have delayed X-ray/optical afterglow ...
... Eiso=4x1052 erg Strong beaming x100 unseen (off beam axis) short GRB! • many more target events for GW! • no regular “GRB”: how to identify? – may have delayed X-ray/optical afterglow ...
