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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.
Källa:B. Saxton (NRAO/AUI/NSF); ALMA (ESO/NAOJ/NRAO); NASA/ESA Hubble
Om bilden
| ID: | eso1633d |
| Typ: | Observation |
| Publiceringsdatum: | 22 september 2016 20:00 |
| Relaterade pressmeddelanden: | eso1633 |
| Storlek: | 1345 x 1279 px |
Om objektet
| Typ: | Early Universe : Cosmology : Morphology : Deep Field |
| Constellation: | Fornax |
| Kategori: | Cosmology |
Skrivbordsunderlägg
Koordinater
| Position (RA): | 3 32 38.59 |
| Position (Dec): | -27° 46' 34.68" |
| Field of view: | 0.39 x 0.29 arcminutes |
| Orientering: | Nord är -0.0° vänster om lodrätt |
Se i WorldWide Telescope:
Färger och filter
| Band | Våglängd | Teleskop |
|---|---|---|
| Synligt ljus B | 435 nm | Hubble Space Telescope ACS |
| Synligt ljus V | 606 nm | Hubble Space Telescope ACS |
| Synligt ljus i | 775 nm | Hubble Space Telescope ACS |
| Synligt ljus I | 814 nm | Hubble Space Telescope ACS |
| Synligt ljus I | 850 nm | Hubble Space Telescope ACS |
| Infrarött Z | 1.05 μm | Hubble Space Telescope WFC3 |
| Infrarött J | 1.25 μm | Hubble Space Telescope WFC3 |
| Infrarött H | 1.6 μm | Hubble Space Telescope WFC3 |
| Millimetervågor 231.2 GHZ | 1.3 mm | Atacama Large Millimeter/submillimeter Array |