NGC1850 as seen with the Very Large Telescope and Hubble

This image shows NGC1850, a cluster of thousands of stars roughly 160 000 light-years away in the Large Magellanic Cloud, a Milky Way neighbour. The reddish filaments surrounding the cluster, made of vast clouds of hydrogen, are believed to be the remnants of supernova explosions. 

The image is an overlay of observations conducted in visible light with ESO’s Very Large Telescope (VLT) and NASA/ESA’s Hubble Space Telescope (HST). The VLT captured the wide field of the image and the filaments, while the central cluster was imaged by the HST.  

Among many stars, this cluster is home to a black hole 11 times as massive as the Sun and to a five-solar-mass star orbiting it. By looking at the star’s orbit, a team of astronomers were able to infer the presence of the black hole, making it the first small black hole outside of our galaxy to be found this way. For this discovery, the team used the Multi Unit Spectroscopic Explorer (MUSE) instrument at the VLT.

Crediti:

ESO, NASA/ESA/R. Gilmozzi/S. Casertano, J. Schmidt

Riguardo l'immagine

Identificazione:eso2116b
Tipo:Osservazione
Data di rilascio:Giovedì 11 Novembre 2021 13:00
Notizie relative:eso2116
Grandezza:3097 x 3093 px

Riguardo all'oggetto

Nome:NGC 1850
Tipo:Local Universe : Nebula : Type : Supernova Remnant
Local Universe : Star : Grouping : Cluster
Constellation:Dorado
Categoria:Star Clusters

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Coordinate

Position (RA):5 8 46.19
Position (Dec):-68° 45' 39.77"
Field of view:6.80 x 6.79 arcminutes
Orientazione:Il Nord è a 33.2° a destra della verticale

Colori e filtri

BandaLunghezza d'ondaTelescopio
Ottico
B
440 nmVery Large Telescope
FORS1
Ottico
B
439 nmHubble Space Telescope
WFPC2
Ottico
V
555 nmHubble Space Telescope
WFPC2
Ottico
V
557 nmVery Large Telescope
FORS1
Ottico
r
675 nmHubble Space Telescope
WFPC2
Ottico
v
569 nmHubble Space Telescope
WFPC2
Ottico
i
791 nmHubble Space Telescope
WFPC2
Ottico
H-alpha
656 nmVery Large Telescope
FORS1
Ottico
H-alpha
656 nmHubble Space Telescope
WFPC2