机构:
INAF, Ist Fis Spazio Interplanetario, Via Fosso Cavaliere 100, I-00133 Rome, ItalyINAF, Ist Fis Spazio Interplanetario, Via Fosso Cavaliere 100, I-00133 Rome, Italy
Spinoglio, Luigi
[1
]
Tommasin, Silvia
论文数: 0引用数: 0
h-index: 0
机构:
INAF, Ist Fis Spazio Interplanetario, Via Fosso Cavaliere 100, I-00133 Rome, ItalyINAF, Ist Fis Spazio Interplanetario, Via Fosso Cavaliere 100, I-00133 Rome, Italy
Tommasin, Silvia
[1
]
Malkan, Matthew A.
论文数: 0引用数: 0
h-index: 0
机构:
Univ Calif Los Angeles, Astron Div, Los Angeles, CA 90095 USAINAF, Ist Fis Spazio Interplanetario, Via Fosso Cavaliere 100, I-00133 Rome, Italy
Malkan, Matthew A.
[2
]
Hainline, Kevin
论文数: 0引用数: 0
h-index: 0
机构:
Univ Calif Los Angeles, Astron Div, Los Angeles, CA 90095 USAINAF, Ist Fis Spazio Interplanetario, Via Fosso Cavaliere 100, I-00133 Rome, Italy
Hainline, Kevin
[2
]
机构:
[1] INAF, Ist Fis Spazio Interplanetario, Via Fosso Cavaliere 100, I-00133 Rome, Italy
[2] Univ Calif Los Angeles, Astron Div, Los Angeles, CA 90095 USA
来源:
STARBURST-AGN CONNECTION
|
2009年
/
408卷
关键词:
SAMPLE;
D O I:
暂无
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
The Spitzer IR,S high resolution spectra of about 90 Seyfert galaxies from the 12 mu m Galaxy Sample are presented and discussed. These represent about 70% of the total complete sample of local Seyfert galaxies. The presence of starburst components in these galaxies can be quantified by powerful mid-IR diagnostics tools (i.e. 11.25 mu m PAH feature equivalent width and the H-2 emission line intensity) as well as the AGN dominance can be measured by specific fine structure line ratios (e.g. [NeV]/[NeII], [NeV]/[SiII], etc.). The observed line ratios are compared to the results of semianalytical models, which can be used to compute the AGN and starburst contributions to the total luminosity of the galaxies.