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Updated: Jul 20, 2026

Spin Saturation Transfer Difference NMR (SSTD NMR): A New Tool to Obtain Kinetic Parameters of Chemical Exchange Processes
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彗星C/1999S4 (LINEAR) のNH3のスピン温度について

H Kawakita1, J Watanabe, H Ando

  • 1Gunma Astronomical Observatory, 6860-86 Nakayama, Takayama, Agatsuma, Gunma 377-0702, Japan. kawakita@astron.pref.gunma.jp

Science (New York, N.Y.)
|November 3, 2001
PubMed
まとめ

彗星C/1999S4 (LINEAR) のアンモニアのオーソ対比比は,土星と天王星の間に氷が形成されたことを示唆しています. これは太陽の星雲についての手がかりを提供します.

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