Search results for " Line: Identification"

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Discovery of hard phase lags in the pulsed emission of GRO J1744-28

2016

We report on the discovery and energy dependence of hard phase lags in the 2.14 Hz pulsed profiles of GRO J1744-28. We used data from XMM-Newton and NuSTAR. We were able to well constrain the lag spectrum with respect to the softest (0.3--2.3 keV) band: the delay shows increasing lag values reaching a maximum delay of $\sim$ 12 ms, between 6 and 6.4 keV. After this maximum, the value of the hard lag drops to 7 ms, followed by a recovery to a plateau at 9 ms for energies above 8 keV. NuSTAR data confirm this trend up to 30 keV, but the measurements are statistically poorer, and therefore, less constraining. The lag-energy pattern up to the discontinuity is well described by a logarithmic fun…

Reverberation010504 meteorology & atmospheric sciencesLogarithmLine: identificationLagAstrophysics::High Energy Astrophysical Phenomenaformation; Line: identification; Stars: individual: (GRO J1744-28); X-rays: binaries; X-rays: general; Astronomy and Astrophysics; Space and Planetary Science [Line]Phase (waves)FOS: Physical sciencesAstrophysicsX-rays: generalPlateau (mathematics)01 natural sciencesSettore FIS/05 - Astronomia E Astrofisica0103 physical sciences010303 astronomy & astrophysics0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsRange (particle radiation)Stars: individual: (GRO J1744-28)Line: formationAstronomy and AstrophysicsRadiusAstronomy and AstrophysicX-rays: binarieDiscontinuity (linguistics)Space and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena
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