Merging galaxies in the distant Universe through a gravitational magnifying glass

The Atacama Large Millimeter/submillimeter Array (ALMA) and many other telescopes on the ground and in space have been used to obtain the best view yet of a collision that took place between two galaxies when the Universe was only half its current age. The astronomers enlisted the help of a galaxy-sized magnifying glass to reveal otherwise invisible detail. These new studies of the galaxy H-ATLAS J142935.3-002836 have shown that this complex and distant object looks like the well-known local galaxy collision, the Antennae Galaxies.

In this picture you can see the foreground galaxy that is doing the lensing, which resembles how our home galaxy, the Milky Way, would appear if seen edge-on. But around this galaxy there is an almost complete ring — the smeared out image of a star-forming galaxy merger far beyond.

This picture combines the views from the NASA/ESA Hubble Space Telescope and the Keck-II telescope on Hawaii (using adaptive optics) along with the ALMA images shown in red. The ALMA data also give information about the motions of the material in the distant merging galaxies and were vital in unravelling the complex object.

Mynd/Myndskeið:

ALMA (ESO/NAOJ/NRAO)/NASA/ESA/W. M. Keck Observatory

Um myndina

Auðkenni:eso1426d
Tegund:Athuganir
Útgáfudagur:Ágú 26, 2014, 18:00 CEST
Tengdar fréttatilkynningar:eso1426
Stærð:612 x 612 px

Um fyrirbærið

Nafn:H-ATLAS J142935.3-002836
Tegund:Early Universe : Galaxy : Type : Interacting
Constellation:Virgo
Flokkur:Cosmology

Myndasnið

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Hnit

Position (RA):14 29 34.79
Position (Dec):0° 28' 33.97"
Field of view:0.11 x 0.11 arcminutes
Stefna:Norður er 10.6° vinstri frá lóðréttu

Litir og síur

TíðnisviðSjónauki
Innrautt
f110w
Hubble Space Telescope
WFC3
Innrautt
H
W. M. Keck Observatory
Innrautt
K
W. M. Keck Observatory
MillímetriAtacama Large Millimeter/submillimeter Array

 

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