THEORETICAL SUPPORT FOR ASSIGNMENT OF X-OGEN TO HCO+ MOLECULAR ION

被引：66

作者：

WAHLGREN, U

LIU, B

PEARSON, PK

SCHAEFER, HF

机构：

[1] IBM CORP,RES LAB,MONTEREY & COTTLE RD,SAN JOSE,CA 95114

[2] UNIV CALIF,DEPT CHEM,BERKELEY,CA 94720

来源：

NATURE-PHYSICAL SCIENCE | 1973年 / 246卷 / 149期

关键词：

D O I：

10.1038/physci246004a0

中图分类号：

Q6 [生物物理学];

学科分类号：

071011 ;

摘要：

引用

页码：4 / 6

页数：3

共 18 条

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[3] UNIDENTIFIED INTERSTELLAR MICROWAVE LINE [J].

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SNYDER, LE .

NATURE, 1970, 228 (5268) :267-&

[4] RADIO SPECTRUM OF H2D+ [J].

DALGARNO, A ;

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ASTROPHYSICAL JOURNAL, 1973, 183 (03) :L131-L133

[5] CHEMIIONIZATION IN INTERSTELLAR CLOUDS [J].

DALGARNO, A ;

OPPENHEIMER, M ;

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[6]

HERZBERG G, 1967, ELECTRONIC SPECTRA P

[7] DEUTERIUM IN ORION NEBULA [J].

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WILSON, RW .

ASTROPHYSICAL JOURNAL, 1973, 179 (02) :L57-L59

[8] CARRIER OF INTERSTELLAR 89.190 GHZ LINE [J].

KLEMPERER, W .

NATURE, 1970, 227 (5264) :1230-+

[9]

Lester, 1971, P C POTENTIAL ENERGY, P87

[10]

LEU MT, 1973, PHYS REV A, V8, P420, DOI 10.1103/PhysRevA.8.420

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