An Imaging Survey of the all (Ultra-)Luminous Infrared Galaxies at in the GOALS Sample
arXiv:1910.10608 · doi:10.3847/1538-4365/ab3bfe
Abstract
This paper presents the result of imaging for luminous infrared galaxies (LIRGs) and ultra-luminous infrared galaxies (ULIRGs). \textbf{It is } a \textbf{complete subsample of Great Observatories All-sky LIRG Survery (GOALS) with }, \textbf{and} consists 148 galaxies with . All the images were carried out using the 2.16-m telescope \textbf{at the Xinglong Station of the} National Astronomy Observatories, Chinese Academy of Sciences\textbf{ (NAOC),} during the year from 2006 to 2009. We obtained pure luminosity for each galaxy and corrected the luminosity for emission, filter transmission and extinction. We also classified these galaxies based on their morphology and interaction. We found that the distribution of star-forming \textbf{regions} in these galaxies is related to this classification. As the merging process advanced, these galaxies tend to have a more compact distribution of star-forming region, higher \textbf{} and warmer IR-color (). \textbf{These} results imply that the degree of dynamical disturbance plays an important role in determining the distribution of star-forming region.
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