Complete active space self-consistent field calculations of the vibrational band strengths for C3

Details Complete active space self-consistent field calculations of the vibrational band strengths for C3 Complete active space self-consistent field calculations of the vibrational band strengths for C3

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...343..554j&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 343, Aug. 1, 1989, p. 554-561. Sponsorship: Naturvetenskapliga Forskningsra

Astronomy and Astrophysics

Astrophysics

26

Carbon Stars, Stellar Atmospheres, Transition Probabilities, Vibrational Spectra, Absorption Spectra, Dipole Moments, Molecular Energy Levels, Opacity

Scientific paper

Complete active space self-consistent calculations of the energy and dipole moment functions were carried out for C3 in its electronic ground state. The absorption coefficient between 0.7 and 75 microns is calculated on the basis of the vibrational band strength of transitions between the 800 lowest states with v less than or equal to (4, 39, 3). In cool carbon stars with a high C/O ratio, C3 is found to be the most prevalent of the known opacity sources.

Affiliated with

Also associated with

No associations

Rating

Complete active space self-consistent field calculations of the vibrational band strengths for C3 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 Complete active space self-consistent field calculations of the vibrational band strengths for C3, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Complete active space self-consistent field calculations of the vibrational band strengths for C3 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1514863