BN/KL complex in the Orion Nebula

This is one of a 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, which is an image ratio of images obtained with TIMMI2 at wavelengths of 10.3 µm and 20.0µm. They show in some detail the structures around the compact sources and the extended thermal emission from the dust. It illustrates how the temperature of the dust in this area varies. The brighter areas are the hotter ones.

Technical information: this image shows the observed 20.0 µm to 10.3 µm brightness ratio and hence the distribution of the colour temperature. The lowest observed ratio corresponds to the highest temperature (a de-reddened colour temperature of about 460K, or +190 °C); it occurs at the location of the BN object .

Créditos:

ESO

Sobre a imagem

Id:eso0113d
Tipo:Observação
Data de divulgação:30 de Março de 2001
Notícias relacionadas:eso0113
Tamanho:479 x 686 px

Sobre o objeto

Nome:Becklin/Neugebauer Complex, BN/KL Complex
Tipo:Milky Way : Nebula : Type : Star Formation
Distância:1400 anos-luz
Categoria:Nebulae

Formatos de imagens

JPEG grande
115,7 KB

Papéis de parede

1024x768
173,8 KB
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320,0 KB
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Cores e filtros

BandaComprimento de ondaTelescópio
Infravermelho
Mid-IR
10 μmESO 3.6-metre telescope
TIMMI2
Infravermelho
Q
20 μmESO 3.6-metre telescope
TIMMI2

Notas: This image shows the observed 20.0 µm to 10.3 µm brightness ratio.