Effective collision strengths for hyperfine structure transitions of possible astrophysical interest

Details Effective collision strengths for hyperfine structure transitions of possible astrophysical interest Effective collision strengths for hyperfine structure transitions of possible astrophysical interest

Nov 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997mnras.292..133z&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 292, Issue 1, pp. 133-135.

Astronomy and Astrophysics

Astronomy

4

Atomic Processes, Line: Formation

Scientific paper

The relativistic distorted wave method described by Sampson & Zhang for calculating collision strengths for hyperfine structure transitions is applied to several H-like and Li-like ions having non-zero nuclear spin and relatively high estimated astrophysical abundances. The collision strengths and effective (Maxwellian-averaged) collision strengths are obtained for a wide range of energies and temperatures.

Affiliated with

Also associated with

No associations

Rating

Effective collision strengths for hyperfine structure transitions of possible astrophysical interest does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Effective collision strengths for hyperfine structure transitions of possible astrophysical interest, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Effective collision strengths for hyperfine structure transitions of possible astrophysical interest will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-924393