scholarly journals Mid‐Infrared Spectral Energy Distribution of NGC 1068 with 0.̋1 Spatial Resolution

2001 ◽  
Vol 557 (2) ◽  
pp. 637-645 ◽  
Author(s):  
Daigo Tomono ◽  
Yoshiyuki Doi ◽  
Tomonori Usuda ◽  
Tetsuo Nishimura
2011 ◽  
Vol 743 (2) ◽  
pp. 163 ◽  
Author(s):  
Ryan A. Lane ◽  
Ohad Shemmer ◽  
Aleksandar M. Diamond-Stanic ◽  
Xiaohui Fan ◽  
Scott F. Anderson ◽  
...  

2004 ◽  
Vol 217 ◽  
pp. 214-215
Author(s):  
T. T. Takeuchi ◽  
H. Hirashita ◽  
T. T. Ishii ◽  
L. K. Hunt ◽  
A. Ferrara

We constructed a model of the infrared spectral energy distribution for very young galaxies by taking into account the dust size distribution in the early stage of galaxy evolution.


2013 ◽  
Vol 764 (2) ◽  
pp. 159 ◽  
Author(s):  
Paulina Lira ◽  
Liza Videla ◽  
Yanling Wu ◽  
Almudena Alonso-Herrero ◽  
David M. Alexander ◽  
...  

2006 ◽  
Vol 2 (S235) ◽  
pp. 180-183
Author(s):  
Vassilis Charmandaris

AbstractI present a brief review of some of the mid-infrared properties of interacting galaxies as these were revealed using observations from the Infrared Space Observatory and Spitzer Space Telescope over the last decade. The variation of the infrared spectral energy distribution in interacting galaxies can be used as an extinction free tracer not only of the location of the star formation activity but also of the physical mechanism dominating their energy production.‡.


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