BN/KL complex in the Orion Nebula

This is one of series of mid-infrared images of the BN/KL complex, a star-forming region deep inside the Orion Nebula, obtained with ESO's Thermal Infrared MultiMode Instrument (TIMMI2), mounted at the Cassegrain focus of the 3.6-m telescope on La Silla. The area is located close to the Trapezium cluster. The dust is more transparent at longer wavelengths and the complex is clearly seen in this image obtained with TIMMI2 at wavelengths of 20.0µm. It shows in some detail the structures around the compact sources and the extended thermal emission from the dust. The brighter areas are the hotter ones.

Technical information: This image shows a similar Q-band (20.0 µm) mosaic, obtained with the same observing procedure. Both photos show diffraction limited structures in a 30 x 42 arcsec 2 sky field. 

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ESO

Om bilden

ID:eso0113c
Typ:Observation
Publiceringsdatum:30 mars 2001
Relaterade pressmeddelanden:eso0113
Storlek:478 x 688 px

Om objektet

Namn:Becklin/Neugebauer Complex, BN/KL Complex
Typ:Milky Way : Nebula : Type : Star Formation
Avstånd:1400 ljusår
Kategori:Nebulae

Bildformat

Originalstorlek
485,8 kB
Stor jpeg
119,2 kB
Skärmstor jpeg
248,6 kB

Skrivbordsunderlägg

1024x768
213,1 kB
1280x1024
297,7 kB
1600x1200
370,3 kB
1920x1200
387,3 kB
2048x1536
505,0 kB

Färger och filter

BandVåglängdTeleskop
Infrarött
Q
20 μmESO 3.6-metre telescope
TIMMI2

 

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