Modelling the pan-spectral energy distributions of Starburst and active galaxies

被引：1

作者：

Dopita, MA ^{[1
]}

Fischera, J ^{[1
]}

Groves, B ^{[1
]}

Sutherland, RS ^{[1
]}

Kewley, LJ ^{[1
]}

Tuffs, R ^{[1
]}

Popescu, C ^{[1
]}

Leitherer, C ^{[1
]}

机构：

[1] Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT, Australia

来源：

INTERPLAY AMONG BLACK HOLES, STARS AND ISM IN GALACTIC NUCLEI | 2004年 / 222期

关键词：

D O I：

10.1017/S1743921304002376

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present results of a self-consistent model of the spectral energy distribution (SED) of starburst galaxies. Two parameters control the IR SED, the mean pressure in the ISM and the destruction timescale of molecular clouds. Adding a simplified AGN spectrum provides mixing lines on IRAS color : color diagrams. This reproduces the observed colors of both AGNs and starbursts.

引用

页码：313 / 314

页数：2

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