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141.
James S. Bolton Martin G. Haehnelt Matteo Viel Robert F. Carswell 《Monthly notices of the Royal Astronomical Society》2006,366(4):1378-1390
The low-density hydrogen and helium in the intergalactic medium (IGM) probed by quasi-stellar object (QSO) absorption lines is sensitive to the amplitude and spectral shape of the metagalactic ultraviolet (UV) background. We use realistic H i and He ii Lyα forest spectra, constructed from state-of-the-art hydrodynamical simulations of a Λ cold dark matter (ΛCDM) universe to confirm the reliability of using line profile fitting techniques to infer the ratio of the metagalactic H i and He ii ionization rates. We further show that the large spatial variations and the anticorrelation with H i absorber density observed in the ratio of the measured He ii to H i column densities can be explained in a model where the H i ionization rate is dominated by the combined UV emission from young star-forming galaxies and QSOs and the He ii ionization rate is dominated by emission from QSOs only. In such a model the large fluctuations in the column density ratio are due to the small number of QSOs expected to contribute at any given point to the He ii ionization rate. A significant contribution to UV emission at the He ii photoelectric edge from hot gas in galaxies and galaxy groups would decrease the expected fluctuations in the column density ratio. Consequently, this model appears difficult to reconcile with the large increase in He ii opacity fluctuations towards higher redshift. Our results further strengthen previous suggestions that observed He ii Lyα forest spectra at z ∼ 2–3.5 probe the tail end of the reionization of He ii by QSOs. 相似文献
142.
Rowan F. Temple Somak Raychaudhury Ian R. Stevens 《Monthly notices of the Royal Astronomical Society》2005,362(2):581-591
We present XMM–Newton observations of NGC 891, a nearby edge-on spiral galaxy. We analyse the extent of the diffuse emission emitted from the disc of the galaxy, and find that it has a single-temperature profile with best-fitting temperature of 0.26 keV, though the fit of a dual-temperature plasma with temperatures of 0.08 and 0.30 keV is also acceptable. There is a considerable amount of diffuse X-ray emission protruding from the disc in the north-west direction out to approximately 6 kpc. We analyse the point-source population using a Chandra observation, using a maximum-likelihood method to find that the slope of the cumulative luminosity function of point sources in the galaxy is −0.77+0.13 −0.1 . Using a sample of other local galaxies, we compare the X-ray and infrared properties of NGC 891 with those of 'normal' and starburst spiral galaxies, and conclude that NGC 891 is most likely a starburst galaxy in a quiescent state. We establish that the diffuse X-ray luminosity of spirals scales with the far-infrared luminosity as L X ∝ L 0.87±0.07 FIR , except for extreme starbursts, and NGC 891 does not fall in the latter category. We study the supernova SN1986J in both XMM–Newton and Chandra observations, and find that the X-ray luminosity has been declining with time more steeply than expected ( L X ∝ t −3 ) . 相似文献
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Aaron Sokasian Tom Abel Lars Hernquist 《Monthly notices of the Royal Astronomical Society》2002,332(3):601-616
We study the reionization of He ii by quasars using a numerical approach that combines 3D radiative transfer calculations with cosmological hydrodynamical simulations. Sources producing the ionizing radiation are selected according to an empirical quasar luminosity function, and are assigned luminosities according to their intrinsic masses. The free parameters associated with this procedure are (1) a universal source lifetime, (2) a minimum mass cut-off, (3) a minimum luminosity cut-off, (4) a solid angle specifying the extent to which radiation is beamed, and (5) a tail-end spectral index for the radiative energy distribution of the sources. We present models in which these parameters are varied, and examine characteristics of the resultant reionization process that distinguish the various cases. In addition, we extract artificial spectra from the simulations and quantify statistical properties of the spectral features in each model.
We find that the most important factor affecting the evolution of He ii reionization is the cumulative number of ionizing photons that are produced by the sources. Comparisons between He ii opacities measured observationally and those obtained by our analysis reveal that the available ranges in plausible values for the parameters provide enough leeway to provide a satisfactory match. However, one property common to all our calculations is that the epoch of He ii reionization must have occurred at a redshift in the range 3≲ z ≲4 . If so, future observational programmes will be able to directly trace the details of the ionization history of helium and to probe the low-density phase of the intergalactic medium during this phase of the evolution of the Universe. 相似文献
We find that the most important factor affecting the evolution of He ii reionization is the cumulative number of ionizing photons that are produced by the sources. Comparisons between He ii opacities measured observationally and those obtained by our analysis reveal that the available ranges in plausible values for the parameters provide enough leeway to provide a satisfactory match. However, one property common to all our calculations is that the epoch of He ii reionization must have occurred at a redshift in the range 3≲ z ≲4 . If so, future observational programmes will be able to directly trace the details of the ionization history of helium and to probe the low-density phase of the intergalactic medium during this phase of the evolution of the Universe. 相似文献
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149.
Roland Diehl 《Experimental Astronomy》1995,6(4):103-108
The imaging telescope COMPTEL aboard the NASA Compton Observatory satellite has been demonstrated to be capable of imaging diffuse emission along the Galactic plane. Here we describe details of the imaging data spaces and methods to model the background. Different methods of imaging analysis are compared. Verification of consistency among these methods is a key factor in overall assessment of diffuse emission results. Source simulations and statistical analysis through the bootstrap method are applied to verify the significances of image structures. 相似文献
150.