MASS AND METAL EJECTION EFFICIENCY IN DISK GALAXIES DRIVEN BY YOUNG STELLAR CLUSTERS OF NUCLEAR STARBURST

被引：0

作者：

Rodriguez-Gonzalez, A. ^{[1
]}

Esquivel, A. ^{[1
]}

Raga, A. C. ^{[1
]}

Colin, P. ^{[2
]}

机构：

[1] Univ Nacl Autonoma Mexico, Inst Ciencias Nucl, Mexico City 04510, DF, Mexico

[2] Univ Nacl Autonoma Mexico, Ctr Radioastron & Astrofis, Morelia 58090, Michoacan, Mexico

来源：

REVISTA MEXICANA DE ASTRONOMIA Y ASTROFISICA | 2011年 / 47卷 / 01期

关键词：

galaxies: starburst; galaxies: star clusters: general; ISM: general; stars:; winds; outflows; SUPER-STAR-CLUSTERS; DWARF GALAXIES; GALACTIC WINDS; INTERSTELLAR-MEDIUM; CHEMICAL EVOLUTION; SIMULATIONS; FEEDBACK; GAS; M82; HYDRODYNAMICS;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present results from models of galactic winds driven by energy injected by nuclear starbursts. The total energy of the starburst is provided by young central stellar clusters and parts of the galactic interstellar medium are pushed out as part of the galactic wind (in some cases the galactic wind contains an important part of the metals produced in the new generation of stars). We have performed adiabatic and radiative 3D N-Body/Smooth Particle Hydrodynamics simulations of galactic winds using the GADGET-2 code. The numerical models cover a wide range of starburst (from similar to 10(2) to similar to 10(7) M-circle dot) and galactic gas masses (from similar to 6 x 10(6) to similar to 10(11) M-circle dot). The concentrated central starburst regions are an efficient; engine for producing the mass and metal loss in galaxies, and also for driving the metal redistribution in galaxies.

引用

页码：113 / 125

页数：13

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