Using rotation measure to search for magnetic fields around galaxies at z ~ 0.5

Publisher： Cambridge University Press

E-ISSN： 1743-9221|11|S321|330-332

ISSN： 1743-9213

Source： Proceedings of the International Astronomical Union, Vol.11, Iss.S321, 2017-03, pp. : 330-332

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

Galaxies Unveiled: Rest-frame UV Clumps at 0.5 < z < 1.5

By  

Proceedings of the International Astronomical Union, Vol. 11, Iss. S321, 2017-03 ,pp. : 364-365

Cambridge University Press

Access to resources Recommend Favorite

Mapping the spatial distribution of star formation in cluster galaxies at z ~ 0.5 with the Grism Lens-Amplified Survey from Space (GLASS)

By  

Proceedings of the International Astronomical Union, Vol. 11, Iss. A29B, 2016-10 ,pp. : 797-800

Cambridge University Press

Access to resources Recommend Favorite

Falling outer rotation curves of star-forming galaxies at 0.7 < z < 2.6 probed with KMOS3D and SINS/zC-SINF

By  

Proceedings of the International Astronomical Union, Vol. 11, Iss. S321, 2017-03 ,pp. : 315-317

Cambridge University Press

Access to resources Recommend Favorite

Using deep images and simulations to trace collisional debris around massive galaxies

By  

Proceedings of the International Astronomical Union, Vol. 11, Iss. S321, 2017-03 ,pp. : 180-182

Cambridge University Press

Access to resources Recommend Favorite

Connecting magnetic fields from sub-galactic scale to clusters of galaxies and beyond with cosmological MHD simulations

By  

Proceedings of the International Astronomical Union, Vol. 11, Iss. A29B, 2016-10 ,pp. : 699-699

Cambridge University Press

Access to resources Recommend Favorite