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Aug 4, 1999 — One way to polarize light is by reflection. Light reflecting off a surface will tend to be polarized, with the direction of polarization (the ...

SAO astronomers Christine Wilson, Glen Petitpas, Daisuke Iono, Alison Peck, Melanie Krips, and Tom Cox, together with ten colleagues, have just published the first in a landmark series of papers on luminous and ultraluminous galaxies using data obtained with SAO's Submillimeter Array (SMA). The SMA allowed the astronomers to measure for the first time the spatial distribution of the warm gas around luminous galaxies' nuclei.

C-Mount Camera Lens Mount ... The CMR(/M) Lens Mount features a 8-32 (M4) tapped mounting hole for post-mounting our C-Mount-compatible camera lenses with our ...

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The primary emphasis is on the simplest type of laser beam, the Gaussian beam. Laser light is normally produced as a highly collimated beam, with the photons in ...

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The scientists reached two surprising conclusions. First, they found that the ratio of the amount of gas to dust is about the same as it is in the Milky Way despite the very different level of star formation activity. Second, they discovered that it is peak gas density, not the peak gas mass, that correlates with the region of maximum brightness. This suggests that the increased rate of star birth is the result of increased availability of molecular gas as the fuel, a conclusion that is in direct contrast to the conventional wisdom that abundant gas increases the efficiency but not the rate of star birth. The new paper, the first in a set that will analyze fourteen nearby galaxies, pioneers new, high spatial resolution diagnostics to provide new insights into these powerful cosmic beacons.

Specialized polarized projector charts are obscured when a patient looks through 1 lens of the polarized glasses (A) but are visible when viewed through the ...

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Ultraluminous infrared galaxies ("ULIRGs") shine with the luminosity of one hundred or more Milky Way galaxies. Their most striking feature, however, is not their tremendous energy output but the fact that nearly all of their radiation is invisible, lying at infrared wavelengths. The source of this energy is intense star formation, and because that activity takes place within dust-filled clouds, the ultraviolet and visible light generated is absorbed by the dust grains and remitted in the infrared.

Halite 2 is a compact, all-fiber femtosecond laser ideal for neuroscience, biophotonics, and microscopy. With 2 W power at 1030 nm, and optional 515 nm second ...

Aug 13, 2024 — Linear polarizers do linear polarization and consist only of one layer. However, because the light remains polarized in a single direction, it ...

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Mar 24, 2022 — The simplest forms of microscopes are very rudimentary, consisting of only one lens and able to only slightly magnify an image.

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Key phrases linking here: pinholing, pinholes, pinhole - Learn more. Details. A glaze defect where tiny holes are present in the fired glaze surface. These ...

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Other articles where pinhole camera is discussed: optics: The pinhole camera: An excellent example of the working of the wavelet theory is found in the ...

ULIRGs are thought to result from collisions between galaxies, and since collisions are common, ULIRGs and the slightly dimmer "luminous infrared galaxies" may represent a period of stellar growth and enrichment that many galaxies (perhaps even our own galaxy) briefly experience, especially at early times in the age of the universe when collisions were common. The connections between galaxy interactions and star formation, however, are poorly understood, in part because the obscuring dust makes it difficult to probe the small nuclei of the two merging galaxies.