Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-08-18
Astronomy and Astrophysics
Astrophysics
11 pages 8 (2 jpg) figures accepted by A&A
Scientific paper
We numerically investigate how fundamental properties of the spectral energy distribution (SED) of a major gas-rich galaxy merger with dusty starburst are determined by the initial orbital configuration of the merger. We found that an infrared luminous galaxy with dusty starburst formed by a nearly retrograde-retrograde merger suffers the most remarkable dust extinction of stellar light and consequently shows very red colors. Considering that a retrograde-retrograde merger does not produce strong and long tidal tails, this result suggests that a luminous infrared galaxy without clear signs of interaction and merging shows very large internal dust extinction and redder colors.These numerical results furthermore imply that the morphology of a luminous infrared galaxy can correlate with the degree of internal dust extinction and thus with the shape of the SED, principally because the morphology of a merger also depends strongly on the initial orbital configuration of the merger.
Bekki Kenji
Shioya Yasihiro
No associations
LandOfFree
On the degree of dust extinction in major mergers does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with On the degree of dust extinction in major mergers, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the degree of dust extinction in major mergers will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-555089