... 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. ...
... RATAN-600 (abbreviated from the RAdio Telescope of the Academy of Sciences) with a 600 metre multielement ring antenna ... The Galaxy: kinematics and dynamics, AGNs, chemical composition, the Local Group . Interstellar medium . ...
... 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 ...
... such as Galactic plane, Galaxy center, closest galaxies, Virgo galaxy cluster, Super ... rest-frame bolometric isotropic energy release and peak energy of the burst is E iso ...
... such as Galactic plane, Galaxy center, closest galaxies, Virgo galaxy cluster, Super ... rest-frame bolometric isotropic energy release and peak energy of the burst is E iso ...
... 25 . Romanyuk I.I., Semenko E.A. Magnetic CP stars in our Galaxy . 32 . ... 119 . Gerth E., Glagolevskij Yu.V. The integral magnetic field of 53 Cam - an effect of ring-like element distribution? . 135 . ...
... 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 ...