Origin of Magnetic Fields in White Dwarfs and Neutron Stars

1971 ◽  
Vol 231 (19) ◽  
pp. 32-33 ◽  
Author(s):  
R. F. O'CONNELL ◽  
K. M. ROUSSEL
2008 ◽  
Author(s):  
Lilia Ferrario ◽  
D. T. Wickramasinghe ◽  
Ye-Fei Yuan ◽  
Xiang-Dong Li ◽  
Dong Lai

1979 ◽  
Vol 53 ◽  
pp. 313-316 ◽  
Author(s):  
J. R. P. Angel

Work in progress at Steward Observatory covering three aspects of magnetism in degenerate dwarfs is reviewed. First, the identification of the Minkowski bands in Grw + 70° 8247 with Zeeman transitions in hydrogen. Second, a determination of field strengths in the more strongly magnetic white dwarfs. Third, some observations and speculations concerning the origin of white dwarf and neutron star magnetic fields.


1973 ◽  
Vol 246 (154) ◽  
pp. 93-93 ◽  
Author(s):  
M. A. RUDERMAN ◽  
P. G. SUTHERLAND

2012 ◽  
Vol 8 (S290) ◽  
pp. 177-178
Author(s):  
A. Taani ◽  
C. M. Zhang ◽  
Y. H. Zhao ◽  
A. Moraghan

AbstractWe present a study of the observational properties of Millisecond Pulsars (MSPs) by way of their magnetic fields, spin periods and masses. These measurements are derived through the scenario of Accretion Induced Collapse (AIC) of white dwarfs (WDs) in stellar binary systems, in order to provide a greater understanding of the characteristics of MSP populations. In addition, we demonstrate a strong evolutionary connection between neutron stars and WDs with binary companions from a stellar binary evolution perspective via the AIC process.


1971 ◽  
Vol 2 (15) ◽  
pp. 815-815 ◽  
Author(s):  
R. F. O'Connell ◽  
K. M. Roussel

2006 ◽  
pp. 265-298
Author(s):  
J. TRÜMPER ◽  
H. RUDER ◽  
M. KLEWS

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