scholarly journals A Multiwavelength Study of the High‐Field Magnetic White Dwarf EUVE J0317−85.5 (=RE J0317−853)

2003 ◽  
Vol 593 (2) ◽  
pp. 1040-1048 ◽  
Author(s):  
Stephane Vennes ◽  
G. D. Schmidt ◽  
L. Ferrario ◽  
D. J. Christian ◽  
D. T. Wickramasinghe ◽  
...  
Keyword(s):  
White Dwarf ◽  
High Field

scholarly journals EUVE J0317 — 855: a rapidly rotating, high-field magnetic white dwarf

1997 ◽  
Vol 292 (2) ◽  
pp. 205-217 ◽  
Author(s):  
Lilia Ferrario ◽  
S. Vennes ◽  
D. T. Wickramasinghe ◽  
J. A. Bailey ◽  
D. J. Christian
Keyword(s):  
White Dwarf ◽  
High Field

Phase‐resolvedHubble Space Telescope/STIS Spectroscopy of the Exposed White Dwarf in the High‐Field Polar AR Ursae Majoris

2001 ◽  
Vol 555 (1) ◽  
pp. 380-392 ◽  
Author(s):  
Boris T. Gansicke ◽  
Gary D. Schmidt ◽  
Stefan Jordan ◽  
Paula Szkody
Keyword(s):  
White Dwarf ◽  
High Field ◽  
Space Telescope

scholarly journals Breaking the 100 MG Barrier: The First High Field Magnetic CV

1997 ◽  
Vol 163 ◽  
pp. 409-412
Author(s):  
Paula Szkody ◽  
Gary D. Schmidt ◽  
Paul S. Smith ◽  
Andrew Silber ◽  
D.W. Hoard ◽  
...  
Keyword(s):  
Magnetic Field ◽  
High Magnetic Field ◽  
White Dwarf ◽  
High Field ◽  
Optical Spectra ◽  
Cataclysmic Variable ◽  
High State ◽  
Optical Photometry ◽  
X Ray ◽  
Cyclotron Emission

AbstractWe present results from IUE and optical spectra, optical photometry and circular polarimetry during high and low states of the highly luminous soft X-ray cataclysmic variable AR UMa that identifies the primary in this system as a white dwarf with a magnetic field of 230 MG. The high magnetic field likely threads accretion blobs all the way from the secondary to below the surface of the white dwarf, resulting in a lack of polarised cyclotron emission and an extreme soft-X-ray luminosity during the high state.

scholarly journals Synthetic Spectra of Magnetic White Dwarfs

1989 ◽  
Vol 114 ◽  
pp. 333-336 ◽  
Author(s):  
Stefan Jordan
Keyword(s):  
Field Strength ◽  
Circular Polarization ◽  
White Dwarf ◽  
High Field ◽  
White Dwarfs ◽  
Polar Field ◽  
Free Electrons ◽  
Synthetic Spectra ◽  
The Continuum

AbstractA new program for the calculation of theoretical spectra and wavelength dependend degrees of the linear and circular polarization for magnetic white dwarfs with hydrogen atmospheres has been developed. The main improvement compared to previous models is a more realistic treatment of the bound-free absorption and of the magnetooptical parameters arising from free electrons in the continuum. For the newly discovered magnetic white dwarf HS 1254+3430 a polar field strength of 18 MG was found. Calculations for the high field object Grw +70°8247 confirms the results of Wickramasinghe and Ferrario (320 MG) but gave a better fit to the spectrum at wavelengths larger than 6200 Å.

A centered dipole model for the high field magnetic white dwarf GRW + 70 deg 8247

1988 ◽  
Vol 327 ◽  
pp. 222 ◽  
Author(s):  
D. T. Wickramasinghe ◽  
Lilia Ferrario
Keyword(s):  
White Dwarf ◽  
High Field ◽  
Dipole Model

scholarly journals The high-field magnetic white dwarf LP790-29: Not a fast rotator

2002 ◽  
Vol 381 (2) ◽  
pp. 487-490 ◽  
Author(s):  
K. Beuermann ◽  
K. Reinsch
Keyword(s):  
White Dwarf ◽  
High Field

Study of segregation in La1.8Sr0.2CuO4 superconductor by STEM-EDS microanalysis

1987 ◽  
Vol 45 ◽  
pp. 54-55
Author(s):  
T. F. Kelly ◽  
P. J. Lee ◽  
E. E. Hellstrom ◽  
D. C. Larbalestier
Keyword(s):  
Rare Earth ◽  
High Field ◽  
Transport Current ◽  
Total Thickness ◽  
New Class ◽  
Ceramic Superconductors ◽  
Current Densities ◽  
Group Ii ◽  
Eds Microanalysis

Recently there has been much excitement over a new class of high Tc (>30 K) ceramic superconductors of the form A1-xBxCuO4-x, where A is a rare earth and B is from Group II. Unfortunately these materials have only been able to support small transport current densities 1-10 A/cm2. It is very desirable to increase these values by 2 to 3 orders of magnitude for useful high field applications. The reason for these small transport currents is as yet unknown. Evidence has, however, been presented for superconducting clusters on a 50-100 nm scale and on a 1-3 μm scale. We therefore planned a detailed TEM and STEM microanalysis study in order to see whether any evidence for the clusters could be seen.A La1.8Sr0.2Cu04 pellet was cut into 1 mm thick slices from which 3 mm discs were cut. The discs were subsequently mechanically ground to 100 μm total thickness and dimpled to 20 μm thickness at the center.

High-field magnetoluminescence of ZnSe quantum wires

1998 ◽  
Vol 184-185 (1-2) ◽  
pp. 339-342 ◽  
Author(s):  
L Parthier
Keyword(s):  
High Field ◽  
Quantum Wires

Star reaches out to white dwarf

Nature ◽  
2005 ◽  
Author(s):  
Roxanne Khamsi
Keyword(s):  
White Dwarf

HIGH FIELD N. M. R. IN Cu(NO3)2 2 1/2 H2O BELOW 1°K

1971 ◽  
Vol 32 (C1) ◽  
pp. C1-943-C1-945
Author(s):  
M. W. van TOL ◽  
M. MATSUURA ◽  
N. J. POULIS
Keyword(s):  
High Field
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