0000000000898079

AUTHOR

C Pinto

showing 3 related works from this author

Unveiling the disc structure in ultraluminous X-ray source NGC 55 ULX-1

2022

Ultraluminous X-ray sources (ULXs) are the most extreme among X-ray binaries in which the compact object, a neutron star or a black hole, accretes matter from the companion star, and exceeds a luminosity of 1039 ergs−1 in the X-ray energy band alone. Despite two decades of studies, it is still not clear whether ULX spectral transitions are due to stochastic variability in the wind or variations in the accretion rate or in the source geometry. The compact object is also unknown for most ULXs. In order to place constraints on to such scenarios and on the structure of the accretion disc, we studied the temporal evolution of the spectral components of the variable source NGC 55 ULX-1. Using rec…

High Energy Astrophysical Phenomena (astro-ph.HE)X-rays: binariesAccretionSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary Scienceaccretion discFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaX-rays: binarieX-rays: individual: NGC 55 ULX-1Accretion discs
researchProduct

A transient ultraluminous X-ray source in NGC 55

2022

Ultraluminous X-ray sources (ULXs) are a class of accreting compact objects with X-ray luminosities above 10$^{39}$ erg s$^{-1}$. The average number of ULXs per galaxy is still not well constrained, especially given the uncertainty on the fraction of ULX transients. Here, we report the identification of a new transient ULX in the galaxy NGC 55 (which we label as ULX-2), thanks to recent XMM-Newton and the Neil Gehrels Swift Observatory observations. This object was previously classified as a transient X-ray source with a luminosity around a few 10$^{38}$ erg s$^{-1}$ in a 2010 XMM-Newton observation. Thanks to new and deeper observations ($\sim$ 130 ks each), we show that the source reaches…

High Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/05 - Astronomia E AstrofisicaaccretionSpace and Planetary Scienceaccretion discFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaX-rays: binarieX-rays: individual: XMMU J001446.81-391123.48
researchProduct

Two-particle transverse momentum correlations in pp and p-Pb collisions at energies available at the CERN Large Hadron Collider

2023

Two-particle transverse momentum differential correlators, recently measured in Pb--Pb collisions at energies available at the CERN Large Hadron Collider (LHC), provide an additional tool to gain insights into particle production mechanisms and infer transport properties, such as the ratio of shear viscosity to entropy density, of the medium created in Pb-Pb collisions. The longitudinal long-range correlations and the large azimuthal anisotropy measured at low transverse momenta in small collision systems, namely pp and p-Pb, at LHC energies resemble manifestations of collective behaviour. This suggests that locally equilibrated matter may be produced in these small collision systems, simil…

two particle correlations large hadron colliderCERN Lablongitudinallarge hadron colliderheavy ion scatteringcollectiveFOS: Physical sciencesanisotropy measuredtransverse momentum correlation[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)transport theoryTeVcorrelation functionNuclear Experiment (nucl-ex)Nuclear ExperimentMonte Carloeffect viscositycorrelation long-rangetwo-particleentropy densityparticle multiplicityCERN LHC Collangular distribution anisotropybroadeningtransverse momentum lowydinfysiikkatwo particle correlations
researchProduct