Chandra and XMM–Newton Observations of H2O Maser Galaxy Mrk 266
DOI: 10.1007/s12036-011-9048-x
Bibcode: 2011JApA...32..179W
Wang, J.; Fan, J. H.; Zhang, J. S.
China
Abstract
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.
2011
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Journal of Astrophysics and Astronomy
XMM-Newton
2