Modelling the thermal X-ray emission around the Galactic centre from colliding Wolf-Rayet winds

Publisher： Cambridge University Press

E-ISSN： 1743-9221|11|S322|39-42

ISSN： 1743-9213

Source： Proceedings of the International Astronomical Union, Vol.11, Iss.S322, 2017-02, pp. : 39-42

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

Clump formation through colliding stellar winds in the Galactic Centre

By  

Proceedings of the International Astronomical Union, Vol. 11, Iss. S322, 2017-02 ,pp. : 204-205

Cambridge University Press

Access to resources Recommend Favorite

Origin of the Galactic Diffuse X-ray Emission: Iron K-Shell Line Diagnostics

By  

Proceedings of the International Astronomical Union, Vol. 11, Iss. S322, 2017-02 ,pp. : 206-207

Cambridge University Press

Access to resources Recommend Favorite

What dominates the X-ray emission of normal galaxies?

By  

Proceedings of the International Astronomical Union, Vol. 11, Iss. A29B, 2016-10 ,pp. : 124-135

Cambridge University Press

Access to resources Recommend Favorite

Intrinsic magnetic discontinuities and solar X‐ray emission

By  

GEOPHYSICAL RESEARCH LETTERS, Vol. 17, Iss. 11, 1990-10 ,pp. : 2055-2058

John Wiley & Sons Inc

Access to resources Recommend Favorite

Evaluation of the structural model for ferrihydrite derived from real-space modelling of high-energy X-ray diffraction data

By Manceau A.  

Clay Minerals, Vol. 44, Iss. 1, 2009-03 ,pp. : 19-34

Mineralogical Society

Access to resources Recommend Favorite