Search results for "stars: individual: MXB 1659−298"

showing 1 items of 1 documents

Broadband spectral analysis of MXB 1659−298 in its soft and hard state

2018

The X-ray transient eclipsing source MXB 1659-298 went into outburst in 1999 and 2015. During these two outbursts the source was observed by XMM-Newton, nuSTAR, and Swift/XRT. Using these observations, we studied the broadband spectrum of the source to constrain the continuum components and to verify whether it had a reflection component, as is observed in other X-ray eclipsing transient sources. We combined the available spectra to study the soft and hard state of the source in the 0.45-55 keV energy range. We report a reflection component in the soft and hard state. The direct emission in the soft state can be modeled with a thermal component originating from the inner accretion disk plus…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)stars: individual: MXB 1659−298010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical Phenomenaaccretion disksFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics01 natural sciencesAccretion (astrophysics)stars: neutronX-rays: binariesAccretion discaccretionSpace and Planetary ScienceAccretion disk0103 physical sciencesBroadbandAstrophysics::Solar and Stellar AstrophysicsSpectral analysisAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]010303 astronomy & astrophysicsStars: individual: MXB 1659-298
researchProduct