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Updated: Jul 22, 2026

Measurement and Analysis of Atomic Hydrogen and Diatomic Molecular AlO, C2, CN, and TiO Spectra Following Laser-induced Optical Breakdown
09:40

Measurement and Analysis of Atomic Hydrogen and Diatomic Molecular AlO, C2, CN, and TiO Spectra Following Laser-induced Optical Breakdown

Published on: February 14, 2014

彗星C/1995 O1 (ヘイル・ボップ) のデュテリウム:DCNの検出

R Meier1, T C Owen, D C Jewitt

  • 1University of Hawaii, Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, USA. meier@uhifa.ifa.hawaii.edu

Science (New York, N.Y.)
|March 28, 1998
PubMed
まとめ

デュテラ化水素シアン化物 (DCN) はヘイル・ボップ彗星で検出され,デュテリウムと水素 (D/H) の比率が高いことが明らかになった. この発見は彗星氷の星間起源を支持し,初期の太陽系形成温度を暗示しています.

キーワード:
NASAの規律 エキゾバイオロジー非NASAのセンターです.

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