UvA - DARE ( Digital Academic Repository ) Polarization - dependent x - ray - absorption spectroscopy of RNi 2 B 2 C ( R = Er to Lu ) : reduced Ni - 3 d occupancy
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UvA - DARE ( Digital Academic Repository ) Multiplet effects in the Ru - L 2 , 3 x - ray absorption spectra of Ru ( IV ) and Ru ( V ) compounds
Disclaimer/Complaints regulations If you believe that digital publication of certain material infringes any of your rights or (privacy) interests, please let the Library know, stating your reasons. In case of a legitimate complaint, the Library will make the material inaccessible and/or remove it from the website. Please Ask the Library: http://uba.uva.nl/en/contact, or a letter to: Library of ...
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Disclaimer/Complaints regulations If you believe that digital publication of certain material infringes any of your rights or (privacy) interests, please let the Library know, stating your reasons. In case of a legitimate complaint, the Library will make the material inaccessible and/or remove it from the website. Please Ask the Library: http://uba.uva.nl/en/contact, or a letter to: Library of ...
متن کاملUvA - DARE ( Digital Academic Repository ) Reservoir spectroscopy of 5 s 5 p 3 P 2 - 5 snd 3 D 1 , 2 , 3 transitions in strontium
Disclaimer/Complaints regulations If you believe that digital publication of certain material infringes any of your rights or (privacy) interests, please let the Library know, stating your reasons. In case of a legitimate complaint, the Library will make the material inaccessible and/or remove it from the website. Please Ask the Library: http://uba.uva.nl/en/contact, or a letter to: Library of ...
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Observations of two unclassified Low Mass X–ray Binaries, X1543–624 and X1556–605, are presented. In the 2– 10 keV band the first of the two sources is a factor of two stronger than the other. Both sources do not show X–ray bursts, dips or eclipses in their X–ray light curves. We find that both spectra are described by a two–component model consisting of emission from a cool accretion disk plus...
متن کاملUvA - DARE ( Digital Academic Repository ) XMM - Newton X - ray study of early type stars in the Carina OB 1 association
Aims. X-ray properties of the stellar population in the Carina OB1 association are examined with special emphasis on early-type stars. Their spectral characteristics provide some clues to understanding the nature of X-ray formation mechanisms in the winds of single and binary early-type stars. Methods. A timing and spectral analysis of five observations with XMM-Newton is performed using variou...
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