S
Stratos Boutloukos
Researcher at University of Maryland, College Park
Publications - 12
Citations - 338
Stratos Boutloukos is an academic researcher from University of Maryland, College Park. The author has contributed to research in topics: Neutron star & Pulsar. The author has an hindex of 6, co-authored 12 publications receiving 333 citations. Previous affiliations of Stratos Boutloukos include University of Illinois at Urbana–Champaign.
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Journal ArticleDOI
A model for the waveform behavior of accreting millisecond x-ray pulsars: nearly aligned magnetic fields and moving emission regions
Frederick K. Lamb,Stratos Boutloukos,Stratos Boutloukos,Sandor Van Wassenhove,Robert T. Chamberlain,Ka Ho Lo,Alexander Clare,Wenfei Yu,M. Coleman Miller +8 more
TL;DR: In this article, the authors investigated a model of the accreting millisecond X-ray pulsars and showed that the magnetic poles of these stars are close to their spin axes, and the gas is channeled along different field lines to different locations on the stellar surface.
Journal ArticleDOI
A model for the waveform behavior of accreting millisecond pulsars: Nearly aligned magnetic fields and moving emission regions
Frederick K. Lamb,Stratos Boutloukos,Sandor Van Wassenhove,Robert T. Chamberlain,Ka Ho Lo,Alexander Clare,Wenfei Yu,M. Coleman Miller +7 more
TL;DR: In this article, the authors investigated a model of the accreting millisecond X-ray pulsars and showed that the magnetic poles of these stars are close to their spin axes, and the gas is channeled along different field lines to different locations on the stellar surface.
Journal ArticleDOI
Origin of intermittent accretion-powered x-ray oscillations in neutron stars with millisecond spin periods
Frederick K. Lamb,Stratos Boutloukos,Stratos Boutloukos,Sandor Van Wassenhove,Robert T. Chamberlain,Ka Ho Lo,M. Coleman Miller +6 more
TL;DR: In this paper, it was shown that moving the emitting area from very close to the spin axis to approximately 10 deg. away can increase the fractional rms amplitude from approx < 0.5% to a few percent, which is easily detectable.
Journal ArticleDOI
Super-Eddington Fluxes During Thermonuclear X-ray Bursts
TL;DR: In this paper, the authors show that the Bose-Einstein spectra of thermonuclear X-ray bursts are not well fit by Planck functions with temperatures so high that they imply a super-Eddington radiative flux at the emitting surface when there is no evidence of photospheric radius expansion.
Journal ArticleDOI
Super-Eddington fluxes during thermonuclear X-ray bursts
TL;DR: In this paper, it was shown that the Bose-Einstein spectra of the Rossi X-ray Timing Explorer (SXT) measurements of the 4U 1820-30 superburst and a long burst from GX 17+2 are well-fit by similar BoseEinstein Spectra with high temperatures and modest chemical potentials.