Results 221 to 230 of about 158,490 (251)
Research on Wind Environment Characteristics of the QiTai Radio Telescope Site Based on Wind Tower Measurements. [PDF]
He F +7 more
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Bimagnon dispersion of La<sub>2</sub>CuO<sub>4</sub> probed by resonant inelastic X-ray scattering. [PDF]
Singh A +8 more
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Massive extended streamers feed high-mass young stars. [PDF]
Olguin FA +15 more
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JWST Observations of Segregated <sup>12</sup>CO<sub>2</sub> and <sup>13</sup>CO<sub>2</sub> Ices in Protostellar Envelopes. [PDF]
Brunken NGC +15 more
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Measuring the magnetic fields in the chromospheres of low-mass stars. [PDF]
Cang T +13 more
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Journal of Quantitative Spectroscopy and Radiative Transfer, 1962
The development of American astronomy over the last quarter century has been chiefly characterized by the construction of larger and larger telescopes. The size and diversity of those covering the visible spectrum have increased steadily over the period.
Lewis M. Branscomb, Richard N. Thomas
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The development of American astronomy over the last quarter century has been chiefly characterized by the construction of larger and larger telescopes. The size and diversity of those covering the visible spectrum have increased steadily over the period.
Lewis M. Branscomb, Richard N. Thomas
openaire +2 more sources
Astrophysical plasma laboratories
Physics World, 1994Almost all of the material in the Universe is in the form of ionized gas or plasma. The interstellar medium is a low-temperature, low-density plasma whilst the interiors of stars are made of extremely hot and dense plasmas. A variety of different plasma conditions can exist within the same star; the centre of the Sun, for example, is at a temperature ...
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Laboratory Astrophysics of Dust
EAS Publications Series, 2011Infrared spectroscopy is the best astronomical tool for studying the composition of cosmic dust. Thanks to the Herschel satellite, dust properties from the FIR to mm wavelength range will be sampled in different astrophysical environments. In the laboratory, the study of the temperature and structural dependence of FIR absorption of cosmic dust analogs
C. Jäger, H. Mutschke, T. Henning
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