Energy spectrum of HeII in a strong magnetic field and bound-bound transition probabilities

Author:

Surmelian G. L.,O'Connell R. F.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference6 articles.

1. Kemp, J. C.: 1970a,Astrophys. J. 162, 169.

2. Kemp, J. C.: 1970b,Astrophys. J. Letters 162, 169.

3. Kemp, J. C., Swedlund, J. B., Landstreet, J. D., and Angel, J.R.P.: 1970,Astrophys. J. Letters 161, 177.

4. Rajagopal, A. K., Chanmugan, G., O'Connell, R. F., and Surmelian, G. L.: 1972,Astrophys. J. 177, 713.

5. Smith, E. R., Henry, R. J. W., Surmelian, G. L., O'Connell, R. F., and Rajagopal, A. K.: 1972,Phys. Rev. (to appear).

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1. Energy Levels of Light Atoms in Strong Magnetic Fields;Advances In Atomic, Molecular, and Optical Physics;2014

2. Polarization line radiative transfer in the atmospheres of magnetic white dwarfs;Astronomische Nachrichten: A Journal on all Fields of Astronomy;1987

3. The spectrum and dipole and quadrupole moments of hydrogen-like and helium-like ions in superstrong fields;Journal of Physics B: Atomic and Molecular Physics;1982-08-28

4. Atoms in high magnetic fields (white dwarfs);Reports on Progress in Physics;1977-02-01

5. The quadratic Zeeman effect in the Caii H and K lines;Astrophysics and Space Science;1975-09

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