ESA - European Space Astronomy Centre
Astrophysikalisches Institut Potsdam
Dr. Karl Remeis-Sternwarte & ECAP
Nagano National College of Technology
Dr. Karl Remeis-Sternwarte & ECAP
Institut fur Astronomie und Astrophysik, University of Tubingen
Institut fur Astronomie und Astrophysik, University of Tubingen
Institut fur Astronomie und Astrophysik, University of Tubingen
Institut fur Astronomie und Astrophysik, University of Tubingen
Institut fur Astronomie und Astrophysik, University of Tubingen
CRESST, University of Maryland Baltimore County
Center for Astrophysics and Space Science, UCSD
Center for Astrophysics and Space Science, UCSD
Center for Astrophysics and Space Science, UCSD
School of Physics and Astronomy, Southampton University
出版者
宇宙航空研究開発機構
出版者（英）
Japan Aerospace Exploration Agency (JAXA)
雑誌名
宇宙航空研究開発機構特別資料:
雑誌名(英)
JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H
巻
JAXA-SP-09-008E
ページ
268 - 269
発行年
2010-02-26
会議概要（会議名, 開催地, 会期, 主催者等）（英）
The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan
抄録（英）
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.
内容記述
著者人数: 15名
内容記述（英）
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
Understanding Cyclotron Lines in the Spectra of Accreting Neutron Stars
64574097.pdf
(128.84KB)
