Dissecting the IRX-β dust attenuation relation: exploring the physical origin of observed variations in galaxies

被引:75
作者
Popping, Gergoe [1 ]
Puglisi, Annagrazia [1 ,2 ]
Norman, Colin A. [3 ,4 ]
机构
[1] European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany
[2] Univ Padua, Dipartimento Fis & Astron, Vicolo Osservatorio 2, I-35122 Padua, Italy
[3] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[4] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
关键词
dust; extinction; galaxies: high redshift; galaxies: ISM; infrared: galaxies; ultraviolet: galaxies; STAR-FORMING GALAXIES; LARGE-MAGELLANIC-CLOUD; ALMA SPECTROSCOPIC SURVEY; GIANT MOLECULAR CLOUDS; INITIAL MASS FUNCTION; ULTRA DEEP FIELD; STARBURST GALAXIES; NEARBY GALAXIES; HIGH-REDSHIFT; LUMINOSITY DENSITY;
D O I
10.1093/mnras/stx2202
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The use of ultraviolet (UV) emission as a tracer of galaxy star formation rate (SFR) is hampered by dust obscuration. The empirical relationship between UV-slope, beta, and the ratio between far-infrared and UV luminosity, IRX, is commonly employed to account for obscured UV emission. We present a simple model that explores the physical origin of variations in the IRX-beta dust attenuation relation. A relative increase in FUV compared to NUV attenuation and an increasing stellar population age cause variations towards red UV-slopes for a fixed IRX. Dust geometry effects (turbulence, dust screen with holes, mixing of stars within the dust screen, two-component dust model) cause variations towards blue UV-slopes. Poor photometric sampling of the UV spectrum causes additional observational variations. We provide an analytic approximation for the IRX-beta relation invoking a subset of the explored physical processes (dust type, stellar population age, turbulence). We discuss observed variations in the IRX-beta relation for local (sub-galactic scales) and high-redshift (normal and dusty star-forming galaxies, galaxies during the epoch of reionization) galaxies in the context of the physical processes explored in our model. High spatial resolution imaging of the UV and sub-mm emission of galaxies can constrain the IRX-beta dust attenuation relation for different galaxy types at different epochs, where different processes causing variations may dominate. These constraints will allow the use of the IRX-beta relation to estimate intrinsic SFRs of galaxies, despite the lack of a universal relation.
引用
收藏
页码:2315 / 2333
页数:19
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