scholarly journals HEAVILY OBSCURED ACTIVE GALACTIC NUCLEI IN HIGH-REDSHIFT LUMINOUS INFRARED GALAXIES

2010 ◽  
Vol 722 (2) ◽  
pp. L238-L243 ◽  
Author(s):  
Ezequiel Treister ◽  
C. Megan Urry ◽  
Kevin Schawinski ◽  
Carolin N. Cardamone ◽  
David B. Sanders
2012 ◽  
Vol 8 (S287) ◽  
pp. 323-332 ◽  
Author(s):  
Andrea Tarchi

AbstractLuminous extragalactic masers are traditionally referred to as the ‘megamasers’. Those produced by water molecules are associated with accretion disks, radio jets, or outflows in the nuclear regions of active galactic nuclei (AGN). The majority of OH maser sources are instead driven by intense star formation in ultra-luminous infrared galaxies, although in a few cases the OH maser emission traces rotating (toroidal or disk) structures around the nuclear engines of AGN. Thus, detailed maser studies provide a fundamental contribution to our knowledge of the main nuclear components of AGN, constitute unique tools to measure geometric distances of host galaxies, and have a great impact on probing the, so far, paradigmatic Unified Model of AGN.


1997 ◽  
Vol 159 ◽  
pp. 312-324
Author(s):  
R. Genzel ◽  
D. Lutz ◽  
E. Sturm ◽  
L. Tacconi ◽  
N. Thatte ◽  
...  

AbstractObservations in the 1 µm to 1 cm wavelength band give important information on the physical processes occurring in and immediately around active galactic nuclei. Concentrating on recent results on ionic, atomic, and molecular emission lines, we discuss as examples the first ISO results on the nature of ultra-luminous infrared galaxies, and near-infrared and millimeter measurements of the central 100 parsecs of the Seyfert 2 galaxy NGC 1068.


1996 ◽  
Vol 470 ◽  
pp. 222 ◽  
Author(s):  
L. M. Shier ◽  
M. J. Rieke ◽  
G. H. Rieke

2020 ◽  
Vol 897 (1) ◽  
pp. 107
Author(s):  
Satoshi Yamada ◽  
Yoshihiro Ueda ◽  
Atsushi Tanimoto ◽  
Saeko Oda ◽  
Masatoshi Imanishi ◽  
...  

1999 ◽  
Vol 186 ◽  
pp. 295-301
Author(s):  
S. Veilleux

A review of recent optical and infrared spectroscopic results on luminous infrared galaxies is presented. The main emphasis is on the ultraluminous objects. Possible correlations with infrared luminosity are identified. These results are used to constrain the nature of the dominant energy source in luminous infrared galaxies, and to test whether these objects may represent an evolutionary phase between starburst galaxies and active galactic nuclei.


2006 ◽  
Vol 644 (1) ◽  
pp. 143-147 ◽  
Author(s):  
K. Brand ◽  
A. Dey ◽  
D. Weedman ◽  
V. Desai ◽  
E. Le Floc’h ◽  
...  

2019 ◽  
Vol 15 (S352) ◽  
pp. 121-122
Author(s):  
A. Plat ◽  
S. Charlot ◽  
G. Bruzual ◽  
A. Feltre ◽  
A. Vidal-Garca ◽  
...  

AbstractTo understand how the nature of the ionizing sources and the leakage of ionizing photons in high-redshift galaxies can be constrained from their emission-line spectra, we compare emission-line models of star-forming galaxies including leakage of ionizing radiation, active galactic nuclei (AGN) and radiative shocks, with observations of galaxies at various redshifts with properties expected to approach those of primeval galaxies.


2005 ◽  
Vol 626 (1) ◽  
pp. 58-69 ◽  
Author(s):  
J. L. Higdon ◽  
S. J. U. Higdon ◽  
D. W. Weedman ◽  
J. R. Houck ◽  
E. Le Floc’h ◽  
...  

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