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ALMA deep view of part of the Hubble Ultra Deep Field
A trove of galaxies, rich in carbon monoxide (indicating star-forming potential) were imaged by ALMA (orange) in the Hubble Ultra Deep Field. 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.
B. Saxton (NRAO/AUI/NSF); ALMA (ESO/NAOJ/NRAO); NASA/ESA Hubble
Om bilden
| ID: | eso1633e |
| Typ: | Observation |
| Publiceringsdatum: | 22 september 2016 20:00 |
| Relaterade pressmeddelanden: | eso1633 |
| Storlek: | 1351 x 1002 px |
Om objektet
| Typ: | Early Universe : Cosmology : Morphology : Deep Field |
| Constellation: | Fornax |
| Kategori: | Cosmology |
Skrivbordsunderlägg
Koordinater
| Position (RA): | 3 32 37.93 |
| Position (Dec): | -27° 46' 33.03" |
| Field of view: | 1.35 x 1.00 arcminutes |
| Orientering: | Nord är 0.0° höger 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 |