Chandra and XMM–Newton Observations of H2O Maser Galaxy Mrk 348

Journal of astrophysics and astronomy

J. S. Zhang1¹  J. Wang¹  Q. Guo² 

[1] School of Physics and Electronic Engineering, Guangzhou University, Guangzhou 510006, China.$$;Hunan University of Humanities, Science and Technology, Loudi 417000, China.$$

关键词: Maser;    galaxies: active;    galaxies: nuclei;    galaxies: individual (Mrk 348);    X-rays: galaxies.;   

DOI  :  

学科分类：天文学(综合)

来源: Indian Academy of Sciences

【 摘 要 】

For H2O megamaser galaxy Mrk 348, Chandra and XMM–Newton data are analysed. The nuclear fitting results of XMM–Newton data suggest the possible existence of a heavily obscured AGN. But the nuclear spectrum extracted from Chandra cannot be well-fitted by the best fitting model for XMM–Newton. Further optimal fitting and discussions are needed.

【 授权许可】

Unknown