Zobrazeno 1 - 10
of 962
pro vyhledávání: '"K. I. Kellermann"'
Autor:
Guenther, David
Publikováno v:
American Scientist, 1987 Sep 01. 75(5), 530-530.
Externí odkaz:
https://www.jstor.org/stable/27854813
Autor:
Salpeter, Edwin E.
Publikováno v:
American Scientist, 1990 Mar 01. 78(2), 166-167.
Externí odkaz:
https://www.jstor.org/stable/29773957
Autor:
M. L. Lister, D. C. Homan, K. I. Kellermann, Y. Y. Kovalev, A. B. Pushkarev, E. Ros, T. Savolainen
Publikováno v:
The Astrophysical Journal, Vol 949, Iss 1, p 34 (2023)
Externí odkaz:
https://doaj.org/article/726e55888ded4d489bdb827208001e2b
Autor:
G. Mann
Publikováno v:
Astronomische Nachrichten: A Journal on all Fields of Astronomy. 311:85-85
Autor:
Wilis D
Publikováno v:
Science (New York, N.Y.) [Science] 1988 Nov 18; Vol. 242 (4881), pp. 1065-6.
Autor:
D, Wilis
Publikováno v:
Science (New York, N.Y.). 242(4881)
Autor:
Leonid Gurvits, Yu. N. Pariiskii, A.A. Konovalenko, Nikolai N. Kolachevsky, Rustam D. Dagkesamanskii, Yurii Yu. Balega, Anatolii M. Cherepashchuk, Lev Zelenyi, Yu. Yu. Kovalev, K. I. Kellermann, Igor D. Novikov, Vladimir Gdalevich Kurt
Publikováno v:
Physics-Uspekhi. 63:622-624
Autor:
D. C. Homan, M. H. Cohen, T. Hovatta, K. I. Kellermann, Y. Y. Kovalev, M. L. Lister, A. V. Popkov, A. B. Pushkarev, E. Ros, T. Savolainen
We present multi-epoch, parsec-scale core brightness temperature observations of 447 AGN jets from the MOJAVE and 2cm Survey programs at 15 GHz from 1994 to 2019. The brightness temperature of each jet over time is characterized by its median value a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::90715a5b01f27a40cad6b35e526fa5e0
Autor:
Derek Wills
Publikováno v:
Science. 242:1065-1066
Autor:
M. L. Lister, D. C. Homan, K. I. Kellermann, Y. Y. Kovalev, A. B. Pushkarev, E. Ros, T. Savolainen
Publikováno v:
The Astrophysical Journal. 923:30
We have analyzed the parsec-scale jet kinematics of 447 bright radio-loud active active galactic nuclei (AGN), based on 15 GHz Very Long Baseline Array (VLBA) data obtained between 1994 August 31 and 2019 August 4. We present new total intensity and