Mid‐infrared Continuum of Starburst Nuclei: Contribution from Hot Large Grains within HiiRegions?

1997 ◽  
Vol 484 (1) ◽  
pp. 222-229 ◽  
Author(s):  
Hideaki Mouri ◽  
Kimiaki Kawara ◽  
Yoshiaki Taniguchi
2004 ◽  
Vol 418 (2) ◽  
pp. 465-473 ◽  
Author(s):  
D. Lutz ◽  
R. Maiolino ◽  
H. W. W. Spoon ◽  
A. F. M. Moorwood

1990 ◽  
Vol 139 ◽  
pp. 118-120
Author(s):  
William K. Rose

OH/IR stars and carbon stars are examples of evolved stars known to lose mass rapidly. In a recent paper (Rose 1987) we have described calculations of infrared continuum radiation from dust in stellar winds from red giants. We compare calculated radiative models with recent infrared measurements and estimate the total contribution of evolved stars to the mid-infrared background radiation observed from the Milky Way and M31.


2009 ◽  
Vol 701 (2) ◽  
pp. 891-914 ◽  
Author(s):  
C. Leipski ◽  
R. Antonucci ◽  
P. Ogle ◽  
D. Whysong

2006 ◽  
Vol 31 (1) ◽  
pp. 71 ◽  
Author(s):  
P. S. Kuo ◽  
K. L. Vodopyanov ◽  
M. M. Fejer ◽  
D. M. Simanovskii ◽  
X. Yu ◽  
...  

2001 ◽  
Vol 365 (3) ◽  
pp. L353-L356 ◽  
Author(s):  
H. W. W. Spoon ◽  
J. V. Keane ◽  
A. G. G. M. Tielens ◽  
D. Lutz ◽  
A. F. M. Moorwood

1998 ◽  
Vol 496 (1) ◽  
pp. 117-132 ◽  
Author(s):  
Dario Fadda ◽  
Giuliano Giuricin ◽  
Gian Luigi Granato ◽  
Donatella Vecchies

2020 ◽  
Vol 28 (25) ◽  
pp. 37903
Author(s):  
Jinwei Zhang ◽  
Qing Wang ◽  
Jingjie Hao ◽  
Heyan Liu ◽  
Jiyong Yao ◽  
...  

2017 ◽  
Vol 7 (2) ◽  
pp. 17180-17180 ◽  
Author(s):  
Jinwei Zhang ◽  
Ka Fai Mak ◽  
Nathalie Nagl ◽  
Marcus Seidel ◽  
Dominik Bauer ◽  
...  

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