Zobrazeno 1 - 6
of 6
pro vyhledávání: '"K. M. Blundell"'
Autor:
M. Georganopoulos, R. M. Sambruna, D. Kazanas, A. N. Cillis, C. C. Cheung, E. S. Perlman, K. M. Blundell, D. S. Davis, Felix A. Aharonian, Werner Hofmann, Frank Rieger
We describe a new, independent method for breaking the deadlock of measuring the cosmologically very important Cosmic Infrared Background. Our method measures the energy density of the Cosmic Infrared Background at the location of radio galaxies by u
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4e4a0e46f402213de72289ad78463a3f
https://doi.org/10.1063/1.3076749
https://doi.org/10.1063/1.3076749
Autor:
P. Alexander, K. M. Blundell
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 267:241-246
Since the discovery of depolarization and spectral asymmetries between the two lobes of radio galaxies and of their correlation with jet-sidedness, there has been debate concerning the origin of these effects. For the majority of sources in which asy
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 259:13P-16P
An image of the nucleus of the giant quasar 4C 74.26 made using very long baseline interferometry at a frequency of 5 GHz shows a one-sided, parsec-scale jet that is well aligned with the 400-kpc jet seen in VLA images. If the jet asymmetry is due to
Publikováno v:
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences. 363:611-612
Autor:
K. M. Blundell, M. Lacy
Publikováno v:
Extragalactic Radio Sources ISBN: 9780792341222
1821+643 is exceptionally bright at optical wavelengths with MB ≈ −27 (Hutchings & Neff 1991), at a redshift of only 0.297. It is however, a radio-quiet quasar (RQQ) as can be demonstrated by considering e.g., the ratio of the luminosity in [Oiii
Publikováno v:
Astrophysical Journal; 6/20/2015, Vol. 806 Issue 2, p1-1, 1p