NGC 1365 central region in infrared light

As seen in this composite image, based on exposures in two infrared-wavebands with the ISAAC multi-mode instrument, the nucleus is also very bright in infrared light. Moreover, this infrared view penetrates further into the obscuring dust to reveal several intriguing, red objects. The reddest two to the N-NE coincide with very compact and intense radio sources which are probably supernova remnants. In others, we are seeing the radiation from dust heated by Super Star Clusters. Combination of 15-min Ks (2.16 µm) and L(3.8 µm) band images made with the Long Wavelength arm plus chopping at the telescope secondary mirror. The field is 17 x 16.5 arcsec 2 with North at the top and East to the left.

Crédit:

ESO

À propos de l'image

Identification:eso9920j
Type:Observation
Date de publication:27 février 1999
Communiqués de presse en rapport:eso9920, eso9911
Taille:2896 x 2777 px

À propos de l'objet

Nom:NGC 1365
Type:Local Universe : Galaxy : Activity : AGN : Seyfert
Distance:60 million années lumière
Catégorie:Nebulae

Image Formats

Grand JPEG
1,3 Mio
JPEG taille écran
202,6 Kio

Zoomable


Fonds d'écran

1024x768
221,1 Kio
1280x1024
332,8 Kio
1600x1200
437,0 Kio
1920x1200
489,8 Kio
2048x1536
640,6 Kio

Couleurs & filtres

DomaineLongueur d'ondeTélescope
Infrarouge
L
3.8 μmVery Large Telescope
ISAAC
Infrarouge
K
2.1 μmVery Large Telescope
ISAAC