A new galaxy Spectral Energy Distribution model with the evolution of dust consistent with chemical evolution. Issue Volume 15:Issue S341(2019) (November 2019)

• Record Type: Journal Article
• Authors: Nishida, Kazuki Y.; Takeuchi, Tsutomu T.; Nagata, Takuma; Asano, Ryosuke S.; Inoue, Akio K.
• Editors: Boquien, Médéric; Lusso, Elisabeta; Gruppioni, Carlotta; Tissera, Patricia
• Is Part Of: Proceedings of the International Astronomical Union. Volume 15:Issue S341(2019)
• Page Start: 152
• Page End: 156
• Publication Date: 2019-11
• Subjects: Panchromatic codes and modeling techniques; Astronomy -- Congresses; Astronomy -- Periodicals; 520
• DOI: 10.1017/S1743921319004794
• Languages: English
• ISSNs: 1743-9213

Abstract

Abstract: The spectral energy distribution (SED) model should treat the evolution of a galaxy from its birth. Dust in galaxies affects the formation and evolution of galaxies in various ways. For example, dust grains scatter and absorb stellar emitted ultraviolet (UV) photons and re-emit the radiation at infrared (IR) wavelengths. In this work, we construct a galaxy SED model based on our dust evolution model (Asano et al. 2013 a, b, 2014) with a rigorous treatment of the chemical evolution. To reduce the computational cost, we adopt mega-grain approximation (MGA; (MGA; Inoue, 2005 ). MGA regards a high density dusty region as a huge size (10 pc) dust grain for calculating dust scattering. In this approximation, we can solve the radiative transfer easily and provide SEDs and attenuation curves of galaxies. This model can be used to fit any galaxy in the wavelength range of 10 nm-3 mm.