A failed galaxy

If you look closely at the faint and fuzzy centre of this picture, you will find a ghostly galaxy — the not-so-spooky-sounding UDG4 — captured using ESO’s VLT Survey Telescope (VST). 

UDG stands for ultra-diffuse galaxy: objects as large as the Milky Way but with 100 – 1000 times fewer stars. These galaxies are extremely faint and lack star-forming gas, which makes them appear almost like a fluffy cosmic cloud, or a smudge in space. Their origins remain uncertain, but astronomers speculate that they could be “failed” galaxies that lost their gas supply early in their lifetimes. 

This image of UDG4 was taken as part of a study from a much larger program, the VST Early-type Galaxy Survey (VEGAS), which aims to investigate very faint structures in galaxy clusters — large groups of many galaxies bound together by gravity. The study, led by Enrichetta Iodice from the Istituto Nazionale di Astrofisica in Italy, has found several UDGs in the Hydra Cluster, but more observations are needed to elucidate their true nature.

Given their flimsy appearance, UDGs can be difficult to spot. Nevertheless, the VST, equipped with its OmegaCAM camera, provides exquisite sensitivity to light, allowing astronomers to study such elusive objects.

Źródło:

ESO/Iodice et al.

O zdjęciu

Identyfikator:potw2122a
Typ:Obserwacje
Data publikacji:31 maja 2021 06:00
Rozmiar:467 x 424 px

O obiekcie

Nazwa:UDG4
Typ:Local Universe : Galaxy
Constellation:Hydra
Kategoria:Galaxies

Formaty zdjęć

Pełen rozmiar
299,6 KB
Wielki JPEG
58,6 KB

Powiększenie


Tapety

1024x768
117,6 KB
1280x1024
159,5 KB
1600x1200
199,3 KB
1920x1200
218,0 KB
2048x1536
270,0 KB

Współrzędne

Pozycja (RA):10 37 2.63
Pozycja (Dec):-27° 12' 15.55"
Pole widzenia:1.63 x 1.48 arcminutes
Orientacja:North is 0.1° lewo of vertical

Kolory i filtry

PasmoDługość faliTeleskop
Optyczny
g
480 nmVLT Survey Telescope
OmegaCAM
Optyczny
r
625 nmVLT Survey Telescope
OmegaCAM
Optyczny
g
480 nmVLT Survey Telescope
OmegaCAM
Optyczny
r
625 nmVLT Survey Telescope
OmegaCAM