scholarly journals High Spatial Resolution Mid‐Infrared Observations of Five Seyfert Galaxies

2004 ◽  
Vol 116 (820) ◽  
pp. 493-496 ◽  
Author(s):  
B. T. Soifer ◽  
G. Neugebauer ◽  
K. Matthews ◽  
E. Egami ◽  
L. Armus
2003 ◽  
Vol 126 (1) ◽  
pp. 143-152 ◽  
Author(s):  
B. T. Soifer ◽  
J. J. Bock ◽  
K. Marsh ◽  
G. Neugebauer ◽  
K. Matthews ◽  
...  

2007 ◽  
Vol 471 (1) ◽  
pp. 173-185 ◽  
Author(s):  
Th. Ratzka ◽  
Ch. Leinert ◽  
Th. Henning ◽  
J. Bouwman ◽  
C. P. Dullemond ◽  
...  

1987 ◽  
Vol 115 ◽  
pp. 71-74
Author(s):  
H. Zinnecker ◽  
A. Chelli ◽  
C. Perrier

High spatial resolution infrared observations (mostly at L, some at K) of several young stars in the ρ Oph dark cloud were obtained with the specklegraph at the ESO 3.6m telescope in Chile in July 1985. Sources included EL29, EL21, EL14 and EL9 (Elias 1978, Table 2), and were all measured in two orthogonal directions, W-E (PA=90°) and N-S (PA=180°). Here we shall present visibility functions for EL29 and EL21 and indicate the spatial structure and dimension of these objects. We refer to Elias (1978, p.468/69) for earlier studies of EL29 and EL21.


2006 ◽  
Vol 2 (S237) ◽  
pp. 476-476
Author(s):  
L. Snijders ◽  
L. J. Kewley ◽  
P. P. van der Werf ◽  
B. R. Brandl

AbstractWe explore the physical characteristics of young stellar clusters in the Antennae by combining recent ground- and space-based mid-infrared observations with a newly developed set of diagnostic diagrams. Spitzer data give an overview of the star-forming regions extending over hundreds of parsecs, showing a dominant diffuse ISM component with a density of 102 cm−3 plus a small fraction of very compact material (106 cm−3). With its higher spatial resolution VISIR gives a close-up view of the latter component. Its emission line ratios suggest that these regions are fundamentally different from local star-forming regions. Instead of having small isolated UCHII regions, as in local star-forming regions, the average density of the medium of the whole region falls in the (ultra)compact regime, exceeding 104 cm−3 over tens of parsecs.


2014 ◽  
Vol 441 (1) ◽  
pp. 630-639 ◽  
Author(s):  
Dinalva A. Sales ◽  
D. Ruschel-Dutra ◽  
M. G. Pastoriza ◽  
R. Riffel ◽  
Cláudia Winge

1975 ◽  
Vol 196 ◽  
pp. L31 ◽  
Author(s):  
P. M. Harvey ◽  
W. F. Hoffmann ◽  
M. F. Campbell

2006 ◽  
Vol 636 (2) ◽  
pp. 932-951 ◽  
Author(s):  
C. McCabe ◽  
A. M. Ghez ◽  
L. Prato ◽  
G. Duchene ◽  
R. S. Fisher ◽  
...  

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