In:
Proceedings of the International Astronomical Union, Cambridge University Press (CUP), Vol. 16, No. S363 ( 2020-06), p. 335-337
Kurzfassung:
We analyzed 39 ks NuSTAR data of Cen X-3 through both orbital- and pulse-phase resolved spectroscopy. Orbital-phase resolved spectra show extrinsic fluctuations due to absorption by surrounding plasma, as the spectral fluctuation mainly emerges below 10 keV. Pulse-phase resolved spectra, on the other hand, show intrinsic fluctuations depending on effectiveness of Comptonization, since the spectrum becomes hard above 10 keV at the pulse peak.
Materialart:
Online-Ressource
ISSN:
1743-9213
,
1743-9221
DOI:
10.1017/S1743921322000242
Sprache:
Englisch
Verlag:
Cambridge University Press (CUP)
Publikationsdatum:
2020
ZDB Id:
2170724-8
SSG:
16,12
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