@inproceedings{oai:jaxa.repo.nii.ac.jp:00005029,
 author = {Kretschmar, Peter and Schonherr, G. and Wilms, J. and Nishimura, O. and Kreykenbohm, I. and Staubert, R. and Klochkov, D. and Santangelo, A. and Caballero, I. and Ferrigno, C. and Pottschmidt, K. and Rothschild, R. and Rivers, E. and Suchy, S. and McBride, V.},
 book = {宇宙航空研究開発機構特別資料:, JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H},
 month = {Feb},
 note = {The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan, Cyclotron lines are formed through transitions of electrons between discrete Landau levels in the accretion columns of accreting neutron stars with strong (B approximately 10(exp 12) G) magnetic fields. We summarize recent results on the formation of the spectral continuum of such systems, describe recent advances in the modeling of the lines based on a modification of the commonly used Monte Carlo approach, and discuss new results on the dependence of the measured cyclotron line energy from the luminosity of transient neutron star systems., 著者人数: 15名, Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science, Number of authors: 15, 資料番号: AA0064574097, レポート番号: JAXA-SP-09-008E},
 pages = {268--269},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Understanding Cyclotron Lines in the Spectra of Accreting Neutron Stars},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}