Effective collision strengths for hyperfine structure transitions of possible astrophysical interest

Monthly Notices of the Royal Astronomical Society

Volumn 292, Issue 1, 1997, Pages 133-135

  Zhang, H L ^a   Sampson, D H ^b  

^a OHIO STATE UNIVERSITY   (United States)

^b PENNSYLVANIA STATE UNIVERSITY   (United States)

Author keywords

Atomic processes; Line: formation

Indexed keywords

ATOMIC PHYSICS;

ATOMIC PROCESS; COLLISION STRENGTH; DISTORTED WAVE METHODS; ENERGY; HYPERFINE STRUCTURE; LI-LIKE IONS; LINE FORMATIONS; NUCLEAR SPINS; RELATIVISTICS; STRUCTURE TRANSITIONS;

ASTROPHYSICS;

EID: 0041983650     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/292.1.133     Document Type: Article

References (6)

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3. Sampson D. H., Zhang H. L., 1997, J. Phys. B, 30, 1449
4. Syunyaev R. A., Churazov E. M., 1984, SvA Lett., 10, 201
5. Zhang H. L., Sampson D. H., 1993, Phys. Rev. A, 47, 208
6. Zhang H. L., Sampson D. H., Mohanty A. K., 1989, Phys. Rev. A, 40, 616