Chandra and XMM-Newton Observations of H2O Maser Galaxy Mrk 266

摘要：

For H2O megamaser galaxy Mrk 266, its Chandra and XMM-Newton data are analyzed here. It shows existence of two obscured nuclei (separation is～5)-Our preferred model, the high energy reflected model can fit the hard component of both nuclei spectra well.

作者: J.Wang J.S.Zhang J.H.Fan

作者单位: Center for Astrophysics,Guangzhou University,Guangzhou 510006,China

会议类型: 国际会议

会议名称: International Conference of Multiwavelength Variability of Blazars(Blazar多波段光变国际学术会议)

会议地点: 广州

会议语种:英文

页码: 179-182

在线出版日期: 2010-09-20（万方平台首次上网日期，不代表论文的发表时间）