Gas halo observed by MUSE surrounding a galaxy merger seen by ALMA

This image shows one of the gas halos newly observed with the MUSE instrument on ESO’s Very Large Telescope superimposed to an older image of a galaxy merger obtained with ALMA. The large-scale halo of hydrogen gas is shown in blue, while the ALMA data is shown in orange. 

The halo is bound to the galaxy, which contains a quasar at its centre. The faint, glowing hydrogen gas in the halo provides the perfect food source for the supermassive black hole at the centre of the quasar. 

The objects in this image are located at redshift 6.2, meaning they are being seen as they were 12.8 billion years ago. While quasars are bright, the gas reservoirs around them are much harder to observe. But MUSE could detect the faint glow of the hydrogen gas in the halos, allowing astronomers to finally reveal the food stashes that power supermassive black holes in the early Universe.

Telif:

ESO/Farina et al.; ALMA (ESO/NAOJ/NRAO), Decarli et al.

Görüntü Hakkında

Kimlik:eso1921a
Tür:Gözlem
Yayın tarihi:19 Aralık 2019 12:00
Bağlantılı bültenler:eso1921
Boyut:1852 x 1550 px

Nesne Hakkında

Tür:Early Universe : Galaxy : Activity : AGN : Quasar
Constellation:Capricornus
Kategori:Cosmology

Görüntü Türleri

Büyük JPEG
176,2 KB

Yaklaştırma


Duvarkağıtları

1024x768
76,9 KB
1280x1024
102,5 KB
1600x1200
138,0 KB
1920x1200
166,1 KB
2048x1536
198,6 KB

Koordinatlar

Position (RA):20 32 10.06
Position (Dec):-21° 14' 2.78"
Field of view:0.16 x 0.13 arcminutes
Yönelim:Kuzey yönü -0.0° sol derece kadar dik konumdan sapma göstermektedir

Renkler & Filtreler

BantTeleskop
Optik
Lyman-alpha
Very Large Telescope
MUSE
Milimetre
CII
Atacama Large Millimeter/submillimeter Array

 

Ayrıca görüntüleyin...