J0806 PowerPoint PPT Presentations

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Spectral%20behaviour%20of%20the%20M7%20like%20NS PowerPoint PPT Presentation
Spectral%20behaviour%20of%20the%20M7%20like%20NS - precession. phase residuals. period: (7.7 /- 0.6) yr. spectral variations ... precession (RBS 1223) Schwope et al. (2005) - grav. waves ...
precession. phase residuals. period: (7.7 /- 0.6) yr. spectral variations ... precession (RBS 1223) Schwope et al. (2005) - grav. waves ...
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PowerPoint Presentation - Isolated Neutron Stars, solid crust PowerPoint PPT Presentation
PowerPoint Presentation - Isolated Neutron Stars, solid crust - angle between LOS and spin axis = angle between magnetic and spin axis ... A grid of 78000 models varying Bquad_i and the LOS, magnetic angles ...
angle between LOS and spin axis = angle between magnetic and spin axis ... A grid of 78000 models varying Bquad_i and the LOS, magnetic angles ...
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X-ray Observations PowerPoint PPT Presentation
X-ray Observations - Page et al. 2004 of Neutron Stars Temperature Limits from X-ray Observations Featureless X-ray Spectra from NSs RX J185635-3754: An Old Isolated NS(?)
Page et al. 2004 of Neutron Stars Temperature Limits from X-ray Observations Featureless X-ray Spectra from NSs RX J185635-3754: An Old Isolated NS(?)
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But I am constant as the Northern Star Of whose truefixed and resting quality There is no fellow in PowerPoint PPT Presentation
But I am constant as the Northern Star Of whose truefixed and resting quality There is no fellow in - But I am constant as the Northern Star Of whose truefixed and resting quality There is no fellow in
But I am constant as the Northern Star Of whose truefixed and resting quality There is no fellow in
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The progeny of binary white dwarf mergers extreme helium stars, R CrB stars and subdwarf B stars PowerPoint PPT Presentation
The progeny of binary white dwarf mergers extreme helium stars, R CrB stars and subdwarf B stars - 24, June 2002. white dwarf mergers. The progeny of binary white dwarf mergers; ... Progeny of WD WD mergers ? Extreme Helium stars. RCrB stars. subdwarf B stars ...
24, June 2002. white dwarf mergers. The progeny of binary white dwarf mergers; ... Progeny of WD WD mergers ? Extreme Helium stars. RCrB stars. subdwarf B stars ...
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Joachim Tr PowerPoint PPT Presentation
Joachim Tr - Radiation radius of the radio-quiet isolated. neutron star RX J1856-3754 ... HZ 43 Her, and Sirius B in the. wavelength band marked by the. dotted lines: ...
Radiation radius of the radio-quiet isolated. neutron star RX J1856-3754 ... HZ 43 Her, and Sirius B in the. wavelength band marked by the. dotted lines: ...
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X-ray Observations PowerPoint PPT Presentation
X-ray Observations - An unidentifed EGRET source contains the. X-ray source in its ... extrapolation of X-ray spectrum to EGRET band. reproduces g-ray spectrum without need for a ...
An unidentifed EGRET source contains the. X-ray source in its ... extrapolation of X-ray spectrum to EGRET band. reproduces g-ray spectrum without need for a ...
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The progeny of binary white dwarf mergers extreme helium stars, R CrB stars and subdwarf B stars PowerPoint PPT Presentation
The progeny of binary white dwarf mergers extreme helium stars, R CrB stars and subdwarf B stars - white dwarf mergers. The progeny of binary white dwarf mergers; ... (Landau & Lifshitz 1958) CO He merger frequency: 4.4 10-3 yr-1 (Neleman's et al. 2001) ...
white dwarf mergers. The progeny of binary white dwarf mergers; ... (Landau & Lifshitz 1958) CO He merger frequency: 4.4 10-3 yr-1 (Neleman's et al. 2001) ...
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HandsOn Astrophysics PowerPoint PPT Presentation
HandsOn Astrophysics - 3) Images replaced with color images; errata fixed. 4) Poster Pages recreated from scratch. 5) Photos, Slides scanned as high resolution tiffs ...
3) Images replaced with color images; errata fixed. 4) Poster Pages recreated from scratch. 5) Photos, Slides scanned as high resolution tiffs ...
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Photometry of V407 Vul and RX J0806'3 1527 PowerPoint PPT Presentation
Photometry of V407 Vul and RX J0806'3 1527 - Ephemeris from Strohmayer (2004) Normalised semi- amplitudes. u' ... Ephemeris from Strohmayer (2005) Normalised semi-amplitudes. u' = 13.4 % g'= 13.6 % i'= 14.8 ...
Ephemeris from Strohmayer (2004) Normalised semi- amplitudes. u' ... Ephemeris from Strohmayer (2005) Normalised semi-amplitudes. u' = 13.4 % g'= 13.6 % i'= 14.8 ...
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