Modeling of Luminous and Ultra Luminous InfraRed Galaxies

被引：0
|
作者：
Bankowicz, Malgorzata [1 ]
Malek, Katarzyna [2 ]
Pollo, Agnieszka [1 ,2 ]
Wierzbicka, Katarzyna [1 ]
机构：
[1] Jagiellonian Univ, Astron Observ, Orla 171, PL-30244 Krakow, Poland
[2] Natl Ctr Nucl Res, Andrzeja Soltana 7, PL-05400 Otwock, Poland
来源：
XXXVII POLISH ASTRONOMICAL SOCIETY MEETING | 2016年 / 3卷
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D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
[Ultra] Luminous InfraRed Galaxies (LIRGs and ULIRGs) have the highest star formation rate among star forming galaxies. Using the infrared (IR) data from the AKARI Deep Field-South (ADF-S) enriched with the data from other instruments, including the Herschel satellite, (8 mu m-10(3) mu m), we model Spectral Energy Distributions (SEDs) of these galaxies. We apply the CMCIRSED model (Caitlin M. Casey InfraRed Spectral Energy Distribution (Casey, 2012)) and the FUV-to-FIR models included in the CIGALE(1) code (Code Investigating GALaxy Emission Noll et al. 2009; Serra et al. 2011) code version v0.5 to estimate stellar mass, dust mass and dust temperatures in [U]LIRGs. We concluded that [U]LIRGs have more dust than normal galaxies but the dust temperature does not change significantly with its mass.
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页码：192 / 194
页数：3
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