Zobrazeno 1 - 10
of 13
pro vyhledávání: '"T. K. Krueger"'
Autor:
S. J. Czyzak, T. K. Krueger
Publikováno v:
Astrophysics and Space Science. 60:99-117
Dipole lengths and dipole velocities have been determined for a series of transitions in N IV, O V and O VI. Some of these transitions are of astrophysical interest and the remainder were computed to give a more complete picture of the transitions in
Autor:
T K Krueger, S J Czyzak
Publikováno v:
Proceedings of the Physical Society. 90:623-627
Extensive calculations are being made of the cross sections for electron impact excitation of the metastable levels of the 3pq (q = 2, 3, 4) configuration. These cross sections are important in the interpretation of gaseous nebulae spectra. Collision
Autor:
S. J. Czyzak, T. K. Krueger
Publikováno v:
Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences. 318:531-539
The formulation for electron collisions with ions in configurations 1s 2 2s 2 2p 2 and 1s 2 2s 2 2p 6 3s 2 3q q has been given in paper I of the present series (Saraph, Seaton & Shemming 1969). The present paper gives results of numerical calculation
Autor:
S. J. Czyzak, T. K. Krueger
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 126:177-194
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 148:361-365
Publikováno v:
Proceedings of the National Academy of Sciences of the United States of America. 66(2)
Diagnostics of low density nebular plasma by means of its forbidden line spectrum require not only a knowledge of certain intensity ratios as a function of its density and temperature but also a knowledge of the occupation numbers of relevant ionic l
Autor:
Michael John Seaton, T. K. Krueger, P. A. P. de Martins, Hannelore E. Saraph, S. J. Czyzak, J. Shemming
Publikováno v:
Planetary Nebulae ISBN: 9789401034753
New calculations of collision strengths are being made for ions in configurations np q , n=2 and 3 and q= 1−5. Wave functions for the entire system are represented by sums over anti-symmetrized products of ion functions and orbitals for the collidi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::66b5b51d79541bbaf58a1685d3b588b0
https://doi.org/10.1007/978-94-010-3473-9_22
https://doi.org/10.1007/978-94-010-3473-9_22
Autor:
S. J. Czyzak, T. K. Krueger
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 130:231-232
Publikováno v:
Proceedings of the Physical Society. 92:1146-1147
Using methods described by Saraph, Seaton and Shemming in 1966, collision strengths have been calculated for the isoelectronic sequences 2p3, 2p4, 3p2 and 3p4.
Publikováno v:
The Astrophysical Journal. 152:765
Solar abundance of Y derived from Y II lines by computing transition probabilities and oscillator strength involving several configurations