摘要
The main constituents of interstellar molecules are ~1, H^(12)C,^(14)N,^(16)O^(32)S,^(28)Si.Within them ,only ^(14)N nucleus has a quadrupole moment.Therefore the spectra of the interstellar molecules with constituent ^(14)N havethe nuclear quadrupole hyperfine splittings which could be resolved by virtueof the advanced techniques in some sources.Measurement of the ratios(R)of the hyperfine(hf)satellite intensities(I)offers important astrophysicalinformations. If the excitation temperatures of the hyperfine satellites
出处
《原子与分子物理学报》
CAS
CSCD
北大核心
1990年第4期1618-1621,共4页
Journal of Atomic and Molecular Physics