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

关键词：

D O I：

暂无

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.

引用

页码：192 / 194

页数：3

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