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10.2183/pjab.92.135 http://scihub22266oqcxt.onion/10.2183/pjab.92.135 C4995313!4995313!27169348     free     free     free       Proc+Jpn+Acad+Ser+B+Phys+Biol+Sci 2016 ; 92 (5): 135-55 Nephropedia Template TP {{tp|p=27169348|t=2016. X-ray studies of neutron stars and their magnetic fields |pdf=|usr=}}{{27169348}} gab.com Text X-ray studies of neutron stars and their magnetic fields JO: Proc Jpn Acad Ser B Phys Biol Sci http://www.kidney.de/pget.php?&tw=1&pmid=27169348 #FOAvip Utilizing results obtained over the past quarter century mainly with Japanese X-ray astronomy satellites, a review is given to some aspects of neutron stars (NSs), with a particular emphasis on the magnetic fields (MFs) of mass-accreting NSs and magnetars. Measurements of electron cyclotron resonance features in binary X-ray pulsars, using the Ginga and Suzaku observatories, clarified that their surface MFs are concentrated in a narrow range of (1?7) × 108 T. Extensive studies of magnetars with Suzaku reinforced their nature as neutron stars with truly strong MFs, and revealed several important clues to their formation, evolution, and physical states. Taking all these results into account, a discussion is made on the origin and evolution of these strong MFs. One possible scenario is that the MF of NSs is a manifestation of some fundamental physics, e.g., neutron spin alignment or chirality violation, and the MF makes transitions from strong to weak states. Twit Text FOAVip X-ray studies of neutron stars and their magnetic fields ????Proc Jpn Acad Ser B Phys Biol Sci http://www.kidney.de/pget.php?&tw=1&pmid=27169348 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=27169348 #FOAvip English Wikipedia <ref>{{Cite pmid|27169348}}</ref> X-ray studies of neutron stars and their magnetic fields #MMPMID27169348 MAKISHIMA K Proc Jpn Acad Ser B Phys Biol Sci 2016[May]; 92 (5): 135-55 PMID27169348show ga Utilizing results obtained over the past quarter century mainly with Japanese X-ray astronomy satellites, a review is given to some aspects of neutron stars (NSs), with a particular emphasis on the magnetic fields (MFs) of mass-accreting NSs and magnetars. Measurements of electron cyclotron resonance features in binary X-ray pulsars, using the Ginga and Suzaku observatories, clarified that their surface MFs are concentrated in a narrow range of (1?7) × 108 T. Extensive studies of magnetars with Suzaku reinforced their nature as neutron stars with truly strong MFs, and revealed several important clues to their formation, evolution, and physical states. Taking all these results into account, a discussion is made on the origin and evolution of these strong MFs. One possible scenario is that the MF of NSs is a manifestation of some fundamental physics, e.g., neutron spin alignment or chirality violation, and the MF makes transitions from strong to weak states. äX-ray studies of neutron stars and their magnetic fields (epmc).pdf DeepDyve Pubget Overpricing