Atomic data relevant to line formation in strongly magnetized white dwarf stars

Details Atomic data relevant to line formation in strongly magnetized white dwarf stars Atomic data relevant to line formation in strongly magnetized white dwarf stars

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.131..595w&link_type=abstract

(IAU, Colloquium on Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments, 93rd, Bamberg, West

Astronomy and Astrophysics

Astrophysics

10

Atomic Energy Levels, Balmer Series, Electron Transitions, Magnetic Stars, Stellar Magnetic Fields, White Dwarf Stars, Magnetic Dipoles, Normal Density Functions, Paschen Series

Scientific paper

Intensities of the Balmer transitions for B of greater than 10 to the 8th Gauss are calculated as a function of field, and strong oscillations of the transition strengths are found which are of importance to the quantitative analysis of the observed spectra of mGrw+70 deg 8247 and PG1031+224, and to the interpretation of polarimetric measurements in these objects. A numerical method in which the wave functions are expanded in terms of spherical harmonics and the radial expansion functions in a complete orthonormal basis set of Laguerre functions with fixed exponents is used in the calculations.

Affiliated with

Also associated with

No associations

Rating

Atomic data relevant to line formation in strongly magnetized white dwarf stars 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 Atomic data relevant to line formation in strongly magnetized white dwarf stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Atomic data relevant to line formation in strongly magnetized white dwarf stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1452578