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Optical SED models of galaxy mergers

Published online by Cambridge University Press:  17 August 2012

Gregory F. Snyder ,
T. J. Cox ,
Christopher C. Hayward ,
Lars Hernquist  and
Patrik Jonsson
Gregory F. Snyder
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden ST, Cambridge, MA 02138 email: [email protected]
T. J. Cox
Affiliation:
Carnegie Observatories, Pasadena, CA
Christopher C. Hayward
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden ST, Cambridge, MA 02138 email: [email protected]
Lars Hernquist
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden ST, Cambridge, MA 02138 email: [email protected]
Patrik Jonsson
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden ST, Cambridge, MA 02138 email: [email protected]
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Abstract

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I discuss recent work in which we construct models of poststarburst galaxies by combining fully three-dimensional hydrodynamic simulations of galaxy mergers with radiative transfer calculations of dust attenuation. The poststarburst signatures can occur shortly after a bright starburst phase in gas-rich mergers, and thus offer a unique opportunity to study the formation of bulges and the effects of feedback. Several additional applications of spatially-resolved spectroscopic models of interacting galaxies include multi-wavelength studies of AGN/starburst diagnostics, mock integral field unit data to interpret the evolution of ULIRGs, and the ‘Green Valley’.

Optical spectra of simulated major gas-rich galaxy mergers can be found at http://www.cfa.harvard.edu/~gsnyder

Keywords

galaxies: evolutiongalaxies:interactionsgalaxies: starburstsmethods:n-body simulationsradiative transfer
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S284: The Spectral Energy Distribution of Galaxies , September 2011 , pp. 193 - 197
Copyright
Copyright © International Astronomical Union 2012

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