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ALMA deep view of part of the Hubble Ultra Deep Field
ALMA surveyed the Hubble Ultra Deep Field, uncovering new details of the star-forming history of the Universe. This close-up image reveals one such galaxy (orange), rich in carbon monoxide, showing it is primed for star formation. The blue features are galaxies imaged by Hubble.
This image is based on the very deep ALMA survey by Manuel Aravena, Fabian Walter and colleagues, covering about one sixth of the full HUDF area.
Crédit:B. Saxton (NRAO/AUI/NSF); ALMA (ESO/NAOJ/NRAO); NASA/ESA Hubble
À propos de l'image
Identification: | eso1633d |
Type: | Observation |
Date de publication: | 22 septembre 2016 20:00 |
Communiqués de presse en rapport: | eso1633 |
Taille: | 1345 x 1279 px |
À propos de l'objet
Type: | Early Universe : Cosmology : Morphology : Deep Field |
Constellation: | Fornax |
Catégorie: | Cosmology |
Fonds d'écran
Coordinates
Position (RA): | 3 32 38.59 |
Position (Dec): | -27° 46' 34.68" |
Field of view: | 0.39 x 0.29 arcminutes |
Orientation: | North is -0.0° left of vertical |
Couleurs & filtres
Domaine | Longueur d'onde | Télescope |
---|---|---|
Visible B | 435 nm | Hubble Space Telescope ACS |
Visible V | 606 nm | Hubble Space Telescope ACS |
Visible i | 775 nm | Hubble Space Telescope ACS |
Visible I | 814 nm | Hubble Space Telescope ACS |
Visible I | 850 nm | Hubble Space Telescope ACS |
Infrarouge Z | 1.05 μm | Hubble Space Telescope WFC3 |
Infrarouge J | 1.25 μm | Hubble Space Telescope WFC3 |
Infrarouge H | 1.6 μm | Hubble Space Telescope WFC3 |
Millimétrique 231.2 GHZ | 1.3 mm | Atacama Large Millimeter/submillimeter Array |