Results 271 to 280 of about 74,003 (312)
Exploring exoplanet dynamics with JWST: Tides, rotation, rings, and moons. [PDF]
Millholland SC, Winn JN.
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Near infra-red absorption spectroscopy for astrophysically significant ions. [PDF]
Dowd K, Doyle E, Dunne P.
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Compact and high-resolution spectrometer via Brillouin integrated circuits. [PDF]
Wang JQ +14 more
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Millimeter-Wave and High-Resolution Infrared Spectroscopy of the Ground and 14 Vibrationally Excited States Lying Below 1300 cm<sup>-1</sup> of Pyrazole. [PDF]
Esselman BJ +7 more
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Experimental and First-Principles Study of an Optimized Cylindrical-Shaped ZnO/g‑C<sub>3</sub>N<sub>4</sub> Heterojunction for Enhanced Adsorption and Photocatalytic Degradation of Methylene Blue Dye. [PDF]
Sinha S +5 more
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Resonance, 1998
The spectrum of light emitted by a star holds deep secrets about it. In particular it gives the temperature of a star. It can also reveal the abundances of elements and whether they are in atomic or ionised states. This part of the series dwells upon some of the riddles associated with stellar spectra and their implications.
openaire +2 more sources
The spectrum of light emitted by a star holds deep secrets about it. In particular it gives the temperature of a star. It can also reveal the abundances of elements and whether they are in atomic or ionised states. This part of the series dwells upon some of the riddles associated with stellar spectra and their implications.
openaire +2 more sources
Astronomical Fourier Transform Spectroscopy Revisited
Annual Review of Astronomy and Astrophysics, 1984The Fourier transform spectrometer (FTS) has joined the ranks of a small number of general purpose, high-performance spectroscopic instruments now available to astronomers. As with any technique, the FTS has advantages and disadvantages in comparison with other current or potential experimental methods.
S. T. Ridgway, J. W. Brault
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Spectroscopy for Amateur Astronomers
2017This accessible guide presents the astrophysical concepts behind astronomical spectroscopy, covering both the theory and the practical elements of recording, processing, analysing and interpreting your spectra. It covers astronomical objects, such as stars, planets, nebulae, novae, supernovae, and events such as eclipses and comet passages.
Marc F. M. Trypsteen, Richard Walker
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