Understanding Cyclotron Lines in the Spectra of Accreting Neutron Stars
dc.contributor.author | Kretschmar, P. | |
dc.contributor.author | Schonherr, G. | |
dc.contributor.author | Wilms, J. | |
dc.contributor.author | Nishimura, O. | |
dc.contributor.author | Kreykenbohm, I. | |
dc.contributor.author | Staubert, R. | |
dc.contributor.author | Klochkov, D. | |
dc.contributor.author | Santangelo, A. | |
dc.contributor.author | Caballero, I. | |
dc.contributor.author | Ferrigno, C. | |
dc.contributor.author | Pottschmidt, Katja | |
dc.contributor.author | Rothschild, R. | |
dc.contributor.author | Rivers, E. | |
dc.contributor.author | Suchy, S. | |
dc.contributor.author | McBride, V. | |
dc.date.accessioned | 2023-09-28T15:46:28Z | |
dc.date.available | 2023-09-28T15:46:28Z | |
dc.date.issued | 2010-02 | |
dc.description.abstract | Cyclotron lines are formed through transitions of electrons between discrete Landau levels in the accretion columns of accreting neutron stars with strong (B ∼ 10¹² G) magnetic fields. We summarize recent results on the formation of the spectral continuum of such systems, describe recent advances in the mod-eling 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. | en_US |
dc.description.uri | https://jaxa.repo.nii.ac.jp/records/5029 | en_US |
dc.format.extent | 2 pages | en_US |
dc.genre | journal articles | en_US |
dc.genre | preprints | en_US |
dc.identifier | doi:10.13016/m2ihtf-uzyy | |
dc.identifier.uri | http://hdl.handle.net/11603/29913 | |
dc.language.iso | en_US | en_US |
dc.relation.isAvailableAt | The University of Maryland, Baltimore County (UMBC) | |
dc.relation.ispartof | UMBC Center for Space Sciences and Technology | |
dc.relation.ispartof | UMBC Physics Department | |
dc.relation.ispartof | UMBC Faculty Collection | |
dc.rights | This item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author. | en_US |
dc.title | Understanding Cyclotron Lines in the Spectra of Accreting Neutron Stars | en_US |
dc.type | Text | en_US |
dcterms.creator | https://orcid.org/0000-0002-4656-6881 | en_US |
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