scholarly journals TheChandra,Hubble Space Telescope, and VLA View of the Circumnuclear Extended Emission in the Narrow Emission Line Galaxy NGC 2110

2006 ◽  
Vol 653 (2) ◽  
pp. 1121-1128 ◽  
Author(s):  
Daniel A. Evans ◽  
Julia C. Lee ◽  
Maria Kamenetska ◽  
Sarah C. Gallagher ◽  
Ralph P. Kraft ◽  
...  
1997 ◽  
Vol 159 ◽  
pp. 386-389
Author(s):  
Ian Evans ◽  
Anuradha Koratkar ◽  
Mark Allen ◽  
Zlatan Tsvetanov ◽  
Michael Dopita

AbstractPhotoionization and shock models of the extended emissionline regions (EELRs) in active galaxies demonstrate that the optical emission lines alone are a poor discriminant of the excitation mechanism. Combining optical and UV data provides a discriminant between nuclear photoionization and autoionizing shock models. Hubble Space Telescope UV spectrophotometry of two Seyferts suggests that the EELRs in these objects are probably photoionized by the nucleus.


2021 ◽  
Vol 923 (2) ◽  
pp. 156
Author(s):  
Y. Sophia Dai ◽  
Matthew M. Malkan ◽  
Harry I. Teplitz ◽  
Claudia Scarlata ◽  
Anahita Alavi ◽  
...  

Abstract We identify a sample of spectroscopically measured emission line galaxy (ELG) Pairs up to z = 1.6 from the Wide Field Camera 3 (WFC3) Infrared Spectroscopic Parallels (WISP) survey. WISP obtained slitless, near-infrared grism spectroscopy along with direct imaging in the J and H bands by observing in the pure-parallel mode with the WFC3 on board the Hubble Space Telescope. From our search of 419 WISP fields covering an area of ∼0.5 deg2, we find 413 ELG pair systems, mostly H α emitters. We then derive reliable star formation rates (SFRs) based on the attenuation-corrected H α fluxes. Compared to isolated galaxies, we find an average SFR enhancement of 40%–65%, which is stronger for major Pairs and Pairs with smaller velocity separations (Δ v < 300 km s−1). Based on the stacked spectra from various subsamples, we study the trends of emission line ratios in pairs, and find a general consistency with enhanced lower ionization lines. We study the pair fraction among ELGs, and find a marginally significant increase with redshift f ∝ (1 + z) α , where the power-law index α = 0.58 ± 0.17 from z ∼ 0.2 to ∼1.6. The fraction of active galactic nuclei is found to be the same in the ELG Pairs as compared to the isolated ELGs.


1985 ◽  
Vol 297 ◽  
pp. 633 ◽  
Author(s):  
K. P. Singh ◽  
G. P. Garmire ◽  
J. Nousek

1987 ◽  
Vol 312 ◽  
pp. 484 ◽  
Author(s):  
K. P. Singh ◽  
G. P. Garmire ◽  
J. Nousek

1996 ◽  
Vol 464 ◽  
pp. 704 ◽  
Author(s):  
Jules P. Halpern ◽  
Michael Eracleous ◽  
Alexei V. Filippenko ◽  
Kaiyou Chen

2007 ◽  
Vol 671 (2) ◽  
pp. 1345-1354 ◽  
Author(s):  
Daniel A. Evans ◽  
Julia C. Lee ◽  
T. Jane Turner ◽  
Kimberly A. Weaver ◽  
Herman L. Marshall

2004 ◽  
Vol 150 (1) ◽  
pp. 165-180 ◽  
Author(s):  
Joanna K. Kuraszkiewicz ◽  
Paul J. Green ◽  
D. Michael Crenshaw ◽  
Jay Dunn ◽  
Karl Forster ◽  
...  

2016 ◽  
Vol 225 (2) ◽  
pp. 27 ◽  
Author(s):  
Ivelina G. Momcheva ◽  
Gabriel B. Brammer ◽  
Pieter G. van Dokkum ◽  
Rosalind E. Skelton ◽  
Katherine E. Whitaker ◽  
...  

1997 ◽  
Vol 291 (1) ◽  
pp. L17-L22 ◽  
Author(s):  
K. Iwasawa ◽  
A. C. Fabian ◽  
W. N. Brandt ◽  
C. S. Crawford ◽  
O. Almaini

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