0000000000643872

AUTHOR

James Reeves

showing 2 related works from this author

XMM-Newton First-Light Observations of the Hickson Galaxy Group 16

2000

This paper presents the XMM-Newton first-light observations of the Hickson-16 compact group of galaxies. Groups are possibly the oldest large-scale structures in the Universe, pre-dating clusters of galaxies, and are highly evolved. This group of small galaxies, at a redshift of 0.0132 (or 80 Mpc) is exceptional in the having the highest concentration of starburst or AGN activity in the nearby Universe. So it is a veritable laboratory for the study of the relationship between galaxy interactions and nuclear activity. Previous optical emission line studies indicated a strong ionising continuum in the galaxies, but its origin, whether from starbursts, or AGN, was unclear. Combined imaging and…

Physicsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Continuum (design consultancy)FOS: Physical sciencesAstronomy and AstrophysicsGalaxies: activeAstrophysicsFirst lightAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxy mergerAstrophysicsGalaxyUniverseRedshiftCompact groupSpace and Planetary ScienceGalaxy groupGalaxies: starburstX-rays: galaxieAstrophysics::Galaxy Astrophysicsmedia_common
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The exceptionally extended flaring activity in the X-ray afterglow of GRB 050730 observed with Swift and XMM-Newton

2007

We present the results of a detailed spectral and temporal analysis of Swift and XMM-Newton observations of the high redshift (z=3.969) GRB 050730. The X-ray afterglow of GRB 050730 was found to decline with time with superimposed intense flaring activity that extended over more than two orders of magnitude in time. Seven distinct re-brightening events starting from 236 s up to 41.2 ks after the burst were observed. The underlying decay of the afterglow was well described by a double broken power-law model with breaks at t_1= 237 +/- 20 s and t_2 = 10.1 (-2.2) (+4.6) ks. The temporal decay slopes before, between and after these breaks were alpha_1 = 2.1 +/- 0.3, alpha_2 = 0.44 (-0.08) (+0.1…

PhysicsAstrophysics (astro-ph)X-rayFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsRedshiftGalaxylaw.inventionAfterglowSpectral evolutionSpace and Planetary SciencelawGamma-ray burstOrder of magnitudeFlare
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