... В частности, для вычисле- ния K-поправки были использованы шаблонные распределения энергии 34 2000 2500 3000 3500 4000 4500 5000 l rest , Е 0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4 Flux density, чJy GRB 970508 host galaxy S5 spectrum c 2 /d.o.f = 0.64/3 Рис. ...
... Figure 4.6 The structure of a typical radio galaxy and the capabilities of radio telescopes. ... interferometry is only able to study the nuclear sources with a brightness of 10 8 - 10 12 K; the rest is not detected ...
... 1 list of about 250 galaxies most of them are RG. ... Fig.1, Redshift record as a function of time for galaxies. ... Now radio galaxies are ahead of QSR- most distant RG has z=4.71, most distant radio ...
... i.e., in the vicinity of our Galaxy), but for an epoch corresponding to red shifts ... all of the presently observable structure in the Universe (galaxies, clusters, etc ...
... of the GRB 000926 host galaxy and BVRI photometry of field galaxies with the SCORPIO ... Host Galaxies: Comparison with the Spectral Energy Distributions of Nearby Galaxies ...
... Photometry of GRB Host Galaxies: Comparison with the Spectral Energy Distributions of Nearby Galaxies and Theoretical Modeling ... 56 . Properties of the host galaxy of the gamma-ray burst 970508 and local star-forming galaxy . Astron. Astrophys., ...
... 7. Distribution of the peak frequencies of the compact components (a) in the rest frame of the observer and (b) in the rest frame of the source. ...