Search results for "Galaxies -X-ray"

showing 2 items of 2 documents

Broad-band spectral analysis of the accreting millisecond X-ray pulsar SAX J1748.9-2021

2016

We analyzed a 115 ks XMM-Newton observation and the stacking of 8 days of INTEGRAL observations, taken during the raise of the 2015 outburst of the accreting millisecond X-ray pulsar SAX J1748.9-2021. The source showed numerous type-I burst episodes during the XMM-Newton observation, and for this reason we studied separately the persistent and burst epochs. We described the persistent emission with a combination of two soft thermal components, a cold thermal Comptonization component (~2 keV) and an additional hard X-ray emission described by a power-law (photon index ~2.3). The continuum components can be associated with an accretion disc, the neutron star (NS) surface and a thermal Compton…

AccretionBinaries - X-rayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesIndividualAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencessymbols.namesakeSettore FIS/05 - Astronomia E AstrofisicaPulsarSAX J1748.9-2021Millisecond pulsarAccretion discs -X-ray0103 physical sciencesAccretion; Accretion discs -X-rays; Binaries - X-rays; Galaxies -X-rays; Individual; SAX J1748.9-2021; Space and Planetary Science; Astronomy and Astrophysics010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSolar massMillisecondAstronomyAstronomy and AstrophysicsAccretion (astrophysics)Neutron starSpace and Planetary ScienceGalaxies -X-rayEddington luminositysymbolsAstrophysics - High Energy Astrophysical PhenomenaX-ray pulsar
researchProduct

A faint outburst of the accreting millisecond X-ray pulsar SAX J1748.9-2021 in NGC 6440

2018

SAX J1748.9-2021 is an accreting X-ray millisecond pulsar observed in outburst five times since its discovery in 1998. In early October 2017, the source started its sixth outburst, which lasted only ~13 days, significantly shorter than the typical 30 days duration of the previous outbursts. It reached a 0.3-70 keV unabsorbed peak luminosity of $\sim3\times10^{36}$ erg/s. This is the weakest outburst ever reported for this source to date. We analyzed almost simultaneous XMM-Newton, NuSTAR and INTEGRAL observations taken during the decaying phase of its 2017 outburst. We found that the spectral properties of SAX J1748.9-2021 are consistent with an absorbed Comptonization plus a blackbody comp…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesLuminositySettore FIS/05 - Astronomia E AstrofisicaMillisecond pulsar0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsAccretion accretion disc010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MillisecondAccretion (meteorology)010308 nuclear & particles physicsAstronomy and AstrophysicsAstronomy and AstrophysicCoronaX-rays: binarieNeutron starX-Rays: galaxies -X-rays: individuals: SAX J1748.9-2021Space and Planetary ScienceElectron temperaturebinaries; X-Rays: galaxies -X-rays: individuals: SAX J1748.9-2021; Astronomy and Astrophysics; Space and Planetary Science [Accretion accretion discs; X-rays]Astrophysics - High Energy Astrophysical PhenomenaX-ray pulsar
researchProduct