Zhao Yongheng; Wei Jianyan; Cheng Linpeng
Source Publicationchinesejournalofastronomyandastrophysics
AbstractIn previous paper we have shown that the soft X-ray spectra of two types of Seyfert 1 galaxies behave statistically differently with increasing intensity. In order to see how the spectrum of blazars changes, we made plots of Hardness Ratio 1 versus Count Rates (HR1-Cts) for 18 blazars observed by ROSAT/PSPC. According to our criteria, ten showed a positive HR1-Cts correlation, two a negative correlation, and the remaining six, no clear correlation. Thus,most blazars of our sample show a hardening spectrum during overall flux increase, though some vary randomly. By investigating the photon index of these objects and different radiation theories, we argue that relative dominance between the synchrotron and inverse Compton emission in the soft X-ray band can well account for the differing spectral behaviours and that the different spectral variations might represent a sequence of synchrotron peaked frequency.
Document Type期刊论文
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Zhao Yongheng,Wei Jianyan,Cheng Linpeng. variabilityofsoftxrayspectralshapeinblazarsobservedbyrosat[J]. chinesejournalofastronomyandastrophysics,2002,002(002):117.
APA Zhao Yongheng,Wei Jianyan,&Cheng Linpeng.(2002).variabilityofsoftxrayspectralshapeinblazarsobservedbyrosat.chinesejournalofastronomyandastrophysics,002(002),117.
MLA Zhao Yongheng,et al."variabilityofsoftxrayspectralshapeinblazarsobservedbyrosat".chinesejournalofastronomyandastrophysics 002.002(2002):117.
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