scholarly journals The Ultraviolet Continuum Emission of Radio Galaxies. I. Description of Sources from the Hubble Space Telescope Archives

1998 ◽  
Vol 114 (2) ◽  
pp. 177-235 ◽  
Author(s):  
Esther L. Zirbel ◽  
Stefi A. Baum



1999 ◽  
Vol 122 (1) ◽  
pp. 81-108 ◽  
Author(s):  
André R. Martel ◽  
Stefi A. Baum ◽  
William B. Sparks ◽  
Eric Wyckoff ◽  
John A. Biretta ◽  
...  


1996 ◽  
Vol 465 (1) ◽  
pp. L5-L8 ◽  
Author(s):  
Stefi A. Baum ◽  
Christopher P. O'Dea ◽  
Sigrid de Koff ◽  
William Sparks, ◽  
Jeffrey J. E. Hayes ◽  
...  


1997 ◽  
Author(s):  
Esther L. Zirbel ◽  
Stefi A. Baum


2014 ◽  
Vol 444 (1) ◽  
pp. 466-475 ◽  
Author(s):  
E. A. Ramírez ◽  
C. N. Tadhunter ◽  
D. Axon ◽  
D. Batcheldor ◽  
C. Packham ◽  
...  


2013 ◽  
Vol 9 (S304) ◽  
pp. 363-370
Author(s):  
Yervant Terzian ◽  
Edward Khachikian

AbstractIt is known that among active galaxies (AG) with strong emission lines (UV-galaxies, Sy1 and Sy2, Markarian and Kazarian galaxies, radio-galaxies, QSOs host galaxies and so on) there is a large percentage of objects with double and multiple (or complex) nuclei. The common sizes of these nuclei are of the order of a few hundred parsecs or kiloparsecs. We shall discuss the results of morphological and spectroscopic observations of a number of “active galaxies” carried out with the 5m Palomar telescope, 2.6m telescope of Ambartsumian Byurakan Astrophysical Observatory, 6m telescope of Special Astrophysical Observatory in Russia, and newer Hubble Space Telescope data.



2019 ◽  
Vol 15 (S341) ◽  
pp. 309-311
Author(s):  
Kaho Sunaga ◽  
Yoichi Tamura ◽  
Minju Lee ◽  
Ken Mawatari ◽  
Akio K. Inoue ◽  
...  

AbstractWe present a 4.7σ detection of the [OIII] 88 μm line in a gravitationally-lensed Lyman break galaxy, RXC J2248-ID3, using the Atacama Large Millimeter/submillimeter Array (ALMA). We did not detect [CII] 158 μm and rest-frame 90 μm dust continuum emission, suggesting that the bulk of the interstellar medium (ISM) is ionized. Our two-component SED model combining the previous Hubble Space Telescope (HST) data and new photometry obtained from Very Large Telescope (VLT), Spitzer and ALMA suggests the presence of young (∼2 Myr) and mature (∼600 Myr) stellar components with the metallicity of Z = 0.2Z⊙. Our findings are in contrast with previous results claiming a very young, metal-poor stellar component.



1996 ◽  
Vol 175 ◽  
pp. 577-580
Author(s):  
W.J.M. Van Breugel

Together with several of my colleagues I have embarked on a comprehensive program to study the radio–aligned restframe UV structures in high redshift radio galaxies (HzRGs) using some of the world's premier optical telescopes: the Hubble Space Telescope for high spatial resolution imaging, and the Keck 10m telescope for high S/N spectropolarimetry. I will discuss some of our latest results from these observations which elucidate, and at the same time obscure, our evolving understanding of HzRGs.





1997 ◽  
Vol 112 (2) ◽  
pp. 415-421 ◽  
Author(s):  
Patrick J. McCarthy ◽  
George K. Miley ◽  
Sigrid de Koff ◽  
Stefi A. Baum ◽  
William B. Sparks ◽  
...  


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