Add to ORKGTo help understand the effects of galaxy interactions on star formation, we analyze Spitzer infrared and GALEX ultraviolet images of the interacting galaxy pair Arp 82 (NGC 2535/6), and compare to a numerical simulation of the interaction. We investigate the UV and IR properties of several star forming regions (clumps). Using the FUV/NUV colors of the clumps we constrain the ages. The 8 micron and 24 micron luminosities are used to estimate the far-infrared luminosities and the star formation rates of the clumps. We investigate possible gradients in the UV and IR colors. See Smith et al. (2006a,b) for global results on our entire interacting sample
International audienceMerger processes play an important role in galaxy formation and evolution. To ...
We construct UV/optical/IR spectral energy distributions for 29 star forming regions in the interact...
A multi-wavelength set of photometric data including UV (GALEX), optical, near-IR, infrared (Spitzer...
International audienceAs part of our Spitzer Spirals, Bridges, and Tails project to help understand ...
As part of our Spitzer Spirals, Bridges, and Tails project to help understand the effects of galaxy ...
As part of our Spitzer Spirals, Bridges, and Tails project to help understand the effects of galaxy ...
Galaxy interactions are known to drive interstellar gas toward the nuclear regions, thus triggering ...
In this study we present GALEX UV, Sloan Digital Sky Survey, and Spitzer infrared imaging, along wit...
We present Spitzer infrared imaging of the peculiar galaxy pair Arp 107 and compare with an optical ...
International audienceWe present Spitzer mid-infrared imaging of a sample of 35 tidally distorted pr...
International audienceWe present Spitzer infrared imaging of the peculiar galaxy pair Arp 107 and co...
Interacting galaxies are known to have higher global rates of star formation on average than normal ...
We use a new stacking technique to obtainmeanmid-IR and far-IR to far-UV flux ratios over the rest-f...
International audienceMerger processes play an important role in galaxy formation and evolution. To ...
We construct UV/optical/IR spectral energy distributions for 29 star forming regions in the interact...
A multi-wavelength set of photometric data including UV (GALEX), optical, near-IR, infrared (Spitzer...
International audienceAs part of our Spitzer Spirals, Bridges, and Tails project to help understand ...
As part of our Spitzer Spirals, Bridges, and Tails project to help understand the effects of galaxy ...
As part of our Spitzer Spirals, Bridges, and Tails project to help understand the effects of galaxy ...
Galaxy interactions are known to drive interstellar gas toward the nuclear regions, thus triggering ...
In this study we present GALEX UV, Sloan Digital Sky Survey, and Spitzer infrared imaging, along wit...
We present Spitzer infrared imaging of the peculiar galaxy pair Arp 107 and compare with an optical ...
International audienceWe present Spitzer mid-infrared imaging of a sample of 35 tidally distorted pr...
International audienceWe present Spitzer infrared imaging of the peculiar galaxy pair Arp 107 and co...
Interacting galaxies are known to have higher global rates of star formation on average than normal ...
We use a new stacking technique to obtainmeanmid-IR and far-IR to far-UV flux ratios over the rest-f...
International audienceMerger processes play an important role in galaxy formation and evolution. To ...
We construct UV/optical/IR spectral energy distributions for 29 star forming regions in the interact...
A multi-wavelength set of photometric data including UV (GALEX), optical, near-IR, infrared (Spitzer...