BIAS
发表于 2025-3-28 17:58:55
Subaru/COMICS Mid-Infrared Spectroscopic Observations of the Dust Plume from Comet 9P/Tempela higher crystalline-to-amorphous silicate ratio than that in the comae of other JF comets, and even that of Oort cloud comets. Near the comet nucleus 3.5 hours after the impact the crystalline-to-amorphous ratio is similar to that of Hale-Bopp coma dust at 0.97 AU.
Hyperalgesia
发表于 2025-3-28 22:04:08
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foliage
发表于 2025-3-29 02:39:03
The Visual Brightness Behavior of Comet 9P/Tempel 1 During 1972–2005 impact time was constructed and it was compared with comet’s water production rate. The photometric peculiarities of comet and long–term evolution of comet’s activity probably will change after impact. Therefore, the results, which are presented in this manuscript, are important.
终点
发表于 2025-3-29 04:53:27
Rebecca Currano,Martin Steinert,Larry Leifer0.06 K km/s for HCN on July 4 after the impact. We did not detect the HCN 1–0 line, 6.7 GHz CH.OH line or 3.4-mm continuum with the Australia Telescope Compact Array (ATCA) on July 4, giving further limits on any small-scale structure due to an outburst.
Heresy
发表于 2025-3-29 11:17:03
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cloture
发表于 2025-3-29 12:03:33
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AFFIX
发表于 2025-3-29 18:55:22
Lutz Gericke,Raja Gumienny,Christoph Meinel impact time was constructed and it was compared with comet’s water production rate. The photometric peculiarities of comet and long–term evolution of comet’s activity probably will change after impact. Therefore, the results, which are presented in this manuscript, are important.
Commonwealth
发表于 2025-3-29 23:15:36
Mapping Design Thinking in the Arab Worldformed initially during the impact. After the first 600 s the time dependence of the intensities of the emission spectra species appear to be consistent with the photochemical formation and destruction of parents and daughters. The spectral changes with time associated with the CH emission appear to
高谈阔论
发表于 2025-3-30 02:40:43
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deficiency
发表于 2025-3-30 07:43:57
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