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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
Um myndina
Auðkenni: | eso1633e |
Tegund: | Athuganir |
Útgáfudagur: | Sep 22, 2016, 20:00 CEST |
Tengdar fréttatilkynningar: | eso1633 |
Stærð: | 1351 x 1002 px |
Um fyrirbærið
Tegund: | Early Universe : Cosmology : Morphology : Deep Field |
Constellation: | Fornax |
Flokkur: | Cosmology |
Bakgrunnsmynd
Hnit
Position (RA): | 3 32 37.93 |
Position (Dec): | -27° 46' 33.03" |
Field of view: | 1.35 x 1.00 arcminutes |
Stefna: | Norður er 0.0° højre frá lóðréttu |
Litir og síur
Tíðnisvið | Bylgjulengd | Sjónauki |
---|---|---|
Sýnilegt B | 435 nm | Hubble Space Telescope ACS |
Sýnilegt V | 606 nm | Hubble Space Telescope ACS |
Sýnilegt i | 775 nm | Hubble Space Telescope ACS |
Sýnilegt I | 814 nm | Hubble Space Telescope ACS |
Sýnilegt I | 850 nm | Hubble Space Telescope ACS |
Innrautt Z | 1.05 μm | Hubble Space Telescope WFC3 |
Innrautt J | 1.25 μm | Hubble Space Telescope WFC3 |
Innrautt H | 1.6 μm | Hubble Space Telescope WFC3 |
Millímetri 231.2 GHZ | 1.3 mm | Atacama Large Millimeter/submillimeter Array |