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.

Telif:

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

Görüntü Hakkında

Kimlik:eso1426d
Tür:Gözlem
Yayın tarihi:26 Ağustos 2014 18:00
Bağlantılı bültenler:eso1426
Boyut:612 x 612 px

Nesne Hakkında

Adı:H-ATLAS J142935.3-002836
Tür:Early Universe : Galaxy : Type : Interacting
Constellation:Virgo
Kategori:Cosmology

Görüntü Türleri

Büyük JPEG
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Koordinatlar

Position (RA):14 29 34.79
Position (Dec):0° 28' 33.97"
Field of view:0.11 x 0.11 arcminutes
Yönelim:Kuzey yönü 10.6° sol derece kadar dik konumdan sapma göstermektedir

Renkler & Filtreler

BantTeleskop
Kırmızı ötesi
f110w
Hubble Space Telescope
WFC3
Kırmızı ötesi
H
W. M. Keck Observatory
Kırmızı ötesi
K
W. M. Keck Observatory
MilimetreAtacama Large Millimeter/submillimeter Array

 

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