scholarly journals Luminosities and star formation rates of galaxies observed with the ultraviolet imaging telescope: A comparison of far-UV, Hα, and far-IR diagnostics

1997 ◽  
Author(s):  
Michael N. Fanelli ◽  
Theodore P. Stecher
1992 ◽  
Vol 395 ◽  
pp. L49 ◽  
Author(s):  
Eric P. Smith ◽  
Robert W. O'Connell ◽  
Ralph C. Bohlin ◽  
Kwang-Ping Cheng ◽  
Robert H. Cornett ◽  
...  

2019 ◽  
Vol 15 (S356) ◽  
pp. 345-347
Author(s):  
Khatun Rubinur ◽  
Mousumi Das ◽  
Preeti Kharb ◽  
P. T. Rahne

AbstractSimulations expect an enhanced star-formation and active galactic nuclei (AGN) activity during galaxy mergers, which can lead to formation of binary/dual AGN. AGN feedback can enhance or suppress star-formation. We have carried out a pilot study of a sample of ˜10 dual nuclei galaxies with AstroSat’s Ultraviolet Imaging Telescope (UVIT). Here, we present the initial results for two sample galaxies (Mrk 739, ESO 509) and deep multi-wavelength data of another galaxy (Mrk 212). UVIT observations have revealed signatures of positive AGN feedback in Mrk 739 and Mrk 212, and negative feedback in ESO 509. Deeper UVIT observations have recently been approved; these will provide better constraints on star-formation as well as AGN feedback in these systems.


1998 ◽  
Vol 507 (1) ◽  
pp. 179-198 ◽  
Author(s):  
Robert S. Hill ◽  
Michael N. Fanelli ◽  
Denise A. Smith ◽  
Ralph C. Bohlin ◽  
Susan G. Neff ◽  
...  

2009 ◽  
Vol 5 (S267) ◽  
pp. 96-102
Author(s):  
Vivienne Wild ◽  
Timothy Heckman ◽  
Paule Sonnentrucker ◽  
Brent Groves ◽  
Lee Armus ◽  
...  

AbstractLarge optical surveys provide an unprecedsCeented census of galaxies in the local Universe, forming an invaluable framework into which more detailed studies of objects can be placed. But how useful are optical surveys for understanding the co-evolution of black holes and galaxies, given their limited wavelength coverage, selection criteria, and depth? Here we present work-in-progress comparing optical and mid-IR diagnostics of three “unusual” low-z populations (luminous Seyferts, dusty Balmer-strong AGN, ULIRGs) with a set of ordinary star-forming galaxies from the SDSS. We address the questions “how well do the mid-IR and optical diagnostics of star formation and AGN strength agree?” and “to what extent do optical surveys allow us to include extreme, dusty, morphologically disturbed galaxies in our ‘complete’ census of BH-galaxy co-evolution?


1993 ◽  
Vol 402 ◽  
pp. L45 ◽  
Author(s):  
Jesse K. Hill ◽  
Susan E. Gessner ◽  
Ralph C. Bohlin ◽  
Kwang-Ping Cheng ◽  
Paul M. N. Hintzen ◽  
...  

2001 ◽  
Vol 548 (2) ◽  
pp. 681-693 ◽  
Author(s):  
Eric F. Bell ◽  
Robert C. Kennicutt, Jr.

2015 ◽  
Vol 11 (A29B) ◽  
pp. 264-264
Author(s):  
Lisa J. Kewley

AbstractI will give an overview of the emission-line diagnostics used for star-forming galaxies. I will review the UV, optical, and IR diagnostics that can be used to yield information about the ISM conditions, star-formation properties, and power sources in GRB hosts, both globally, and with spatially-resolved data. I will discuss wide integral field spectroscopy and AO-led integral field spectroscopy on current and future telescopes, focusing on the insights to be gained on the properties of GRB sites.


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