星系間交互作用在星系演化的重要性

The Role of Major Galaxy Interactions in Galaxy Evolution Since Redshift z ~ 1

林俐暉(Lihwai Lin)

指導教授 ： 闕志鴻

國立臺灣大學/理學院/物理研究所/博士(2006年)

https://doi.org/10.6342/NTU.2006.02979

摘要

無資料

關鍵字

星系 ； 交互作用 ； 紅外線

並列摘要

We present the close, kinematic pair fraction and merger rate up to redshift $z sim 1.2$ for a large sample of
galaxies observed by the DEEP2 Redshift Survey. The effect of the galaxy interactions/mergers has also been
addressed by studying the infrared luminosity to the stellar mass ratios speir for $sim 100$ galaxies using images
taken by the $Hubble$ $Space$ $Telescope$ Advanced Camera for Surveys in $V$ and $I$ and $Spitzer$ MIPS in 24m.
Assuming a mild luminosity evolution, the number of companions per luminous galaxy is found to evolve as
$(1+z)^{m}$, with $m= 0.51pm0.28$. Our results imply that only $9\%$ of present-day $L^{*}$ galaxies have undergone
major mergers since $zsim1.2$ and that the average major merger rate is about $4 imes 10^{-4}$ $h^{3}$ Mpc$^{-3}$
Gyr$^{-1}$ for $z sim 0.5 - 1.2$. When dividing the galaxies into blue and red colors, the evolution index $m$
remains similar for blue-blue pairs while $m$ becomes negative for red galaxies. The evolution trend for different
types of galaxies can be explained by the change of galaxy number density and clustering properties over cosmic
time. At fixed stellar mass (sm) the median infrared luminosity (lir) among merging galaxies and close pairs of
blue galaxies is twice (1.9$pm$0.4) that of control pairs drawn from isolated blue galaxies. Enhancement declines
with galaxy separation, being strongest in close pairs and mergers and weaker in wide pairs compared to the control
sample. At $overline{z} sim 0.9$, $7.1pm4.3\%$ of massive interacting galaxies (sm $>$ $2 imes10^{10}
M_{odot}$) are found to be ULIRGs, compared to $2.6pm0.7\%$ in the control sample. The large spread of speir
among interacting galaxies suggests that this enhancement may depend on the merger stage as well as other as yet
unidentified factors (e.g., galaxy structure, mass ratio, orbital characteristics, presence of AGN or bar). The
contribution of interacting systems to the total IR luminosity density is moderate ($leq 36\%$).

並列關鍵字

galaxies:interactions ； galaxies:evolution ； infrared:galaxies

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