MAJOR-MERGER GALAXY PAIRS AT Z = 0: DUST PROPERTIES AND COMPANION MORPHOLOGY

ABSTRACT We present an analysis of dust properties of a sample of close major-merger galaxy pairs selected by Ks magnitude and redshift. The pairs represent the two populations of spiral-spiral (S+S) and mixed morphology spiral-elliptical (S+E). The Code Investigating GALaxy Emission software is use...

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Veröffentlicht in:	The Astrophysical journal 2016-10, Vol.829 (2), p.78
Hauptverfasser:	Domingue, Donovan L., Cao, Chen, Xu, C. Kevin, Jarrett, Thomas H., Ronca, Joseph, Hill, Emily, Jacques, Allison
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY COSMIC DUST DISSOCIATION Dust Dust composition Emission analysis EMISSION SPECTRA FLUX DENSITY GALACTIC EVOLUTION GALAXIES galaxies: evolution galaxies: interactions galaxies: ISM galaxies: spiral Infrared astronomy INFRARED SURVEYS INTERACTIONS Interstellar radiation Morphology Photodissociation PHOTOLYSIS POLYCYCLIC AROMATIC HYDROCARBONS Properties (attributes) Radiation RED SHIFT Sky surveys (astronomy) SPACE Space telescopes Spiral galaxies Spirals STANDARD MODEL Star & galaxy formation Star formation STARS Stars & galaxies TELESCOPES TORQUE Wide-field Infrared Survey Explorer
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