Reflection Nebulae

2016 ◽  
pp. 247-264
Author(s):  
Martin Griffiths
Keyword(s):  
Reflection Nebulae

Physical parameters of reflection nebulae in the galaxy

1989 ◽  
Vol 156 (1-2) ◽  
pp. 51-56
Author(s):  
M. Centuri�n ◽  
G. Vladilo
Keyword(s):  
Physical Parameters ◽  
The Galaxy ◽  
Reflection Nebulae

Erratum to: Reflection Nebulae

1992 ◽  
pp. 945-945
Author(s):  
Kenneth R. Lang
Keyword(s):  
Reflection Nebulae

Reflection Nebulae, Non-Equilibrium Thermal Emission, and IRAS

1986 ◽  
pp. 261-262
Author(s):  
K. Sellgren ◽  
L. J. Allamandola ◽  
J. D. Bregman ◽  
M. W. Werner ◽  
D. H. Wooden
Keyword(s):  
Thermal Emission ◽  
Reflection Nebulae ◽  
Non Equilibrium

scholarly journals ISO Observations of Compact HII Regions in the Large Magellanic Cloud

1999 ◽  
Vol 190 ◽  
pp. 377-378
Author(s):  
A. Moneti ◽  
R. J. Laureijs ◽  
J.M. van der Hulst ◽  
F. Israel ◽  
P.P. van der Werf
Keyword(s):  
Star Formation ◽  
Hii Regions ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Magellanic Clouds ◽  
First Results ◽  
Reflection Nebulae ◽  
Compact Hii Regions

With the detection of strong PAH features and H2 emission in selected knots of the N159, N11A, and 30 Dor regions in the LMC, we present the first results of a study that is part of a coordinated Guaranteed Time ISO programme to investigate star formation in the Magellanic Clouds. The PAH features have different ratios than the ones in Galactic reflection nebulae.

scholarly journals Oh Observations Near the Reflection Nebulae Ngc 2068 and Ngc 2071

1974 ◽  
Vol 60 ◽  
pp. 301-302
Author(s):  
L. E. B. Johansson ◽  
B. Höglund ◽  
A. Winnberg ◽  
Nguyen-Q-Rieu ◽  
W. M. Goss
Keyword(s):  
Dust Cloud ◽  
T Tauri Stars ◽  
Emission Lines ◽  
Class I ◽  
Reflection Nebula ◽  
Cosmic Background ◽  
T Tauri ◽  
Reflection Nebulae

Narrow OH emission lines at 1667 MHz, apparently from a Class I source, have been observed near the reflection nebula NGC 2071. The region contains many T Tauri stars. OH emission corresponding to the dust cloud north and east of NGC 2024 is also seen. At 1720 MHz the dust cloud component appears in absorption; presumably the isotropic 2.7 K cosmic background is being absorbed.

Observations of lam 4430 in reflection nebulae.

1971 ◽  
Vol 76 ◽  
pp. 264 ◽  
Author(s):  
M. F. Hearn
Keyword(s):  
Reflection Nebulae
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