贵族 发表于 2025-3-23 10:06:56

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伪书 发表于 2025-3-23 14:55:19

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小样他闲聊 发表于 2025-3-23 21:22:40

Isotope Fractionation in Interstellar Moleculesal electron density and CO abundance — can be derived from the fractionation process producing the enhanced DCO./HCO. ratio. Possible fractionation reactions for isotopes of other elements (oxygen, sulfur) are mentioned briefly.

Apraxia 发表于 2025-3-24 00:03:17

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arthroplasty 发表于 2025-3-24 05:12:08

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Customary 发表于 2025-3-24 07:06:00

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尖酸一点 发表于 2025-3-24 12:35:28

https://doi.org/10.1007/978-3-662-52815-0Mahoney, McCutcheon and Shuter (1976) reported observations of the J = 1 → 0 transition of three isotopes of CO in the dust cloud Lynds 134 using the 4.6 m telescope at Aerospace Corporation. Here we discuss a new observation of .C.O and consider further the question of the ratio .C.O/.C.O across the dust cloud.

HEED 发表于 2025-3-24 16:35:49

https://doi.org/10.1007/978-3-662-68674-4To derive abundance ratios from measured line intensities several fundamental assumptions are usually made. The two most important of these are that:

懒洋洋 发表于 2025-3-24 21:42:56

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奇思怪想 发表于 2025-3-25 02:13:09

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查看完整版本: Titlebook: CNO Isotopes in Astrophysics; Proceedings of a Spe Jean Audouze Conference proceedings 1977 D. Reidel Publishing Company, Dordrecht,Holland