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The top documents tagged [strong absorption lines]
Terahertz_An introduction
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Post-SM4 Sensitivity Calibration of the STIS Echelle Modes Azalee Bostroem With help from: Ralph Bohlin, Alessandra Aloisi, Charles Proffitt, Kenneth Hart,
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Stellar Temperatures Wien’s law works perfectly for objects with Planck spectra. Stars don’t quite have Planck-like spectra. UV Blue Green Red Infrared
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The Sun
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Final review Feedback Processes in one system influences processes in another interconnected system by exchange of matter and energy. Positive Feedback:
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Stellar Temperatures
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Kennicutt (1992) Galaxies are shown in order of increasing Hubble type from top to bottom. Continuum: sharp break and rise after H and K lines (hence brighter
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The Sun Our Star Please press “1” to test your transmitter
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