Star-forming region NGC 346

This new portrait of the bright star-forming region NGC 346, in which different wavelengths of light swirl together like watercolours, reveals new information about how stars form. NGC 346 is located 210,000 light-years away in the Small Magellanic Cloud, a neighbouring dwarf galaxy of the Milky Way. The image is based on data from ESA XMM-Newton (X-rays; blue), ESO's New Technology Telescope (visible light; green), and NASA's Spitzer (infrared; red). The infrared light shows cold dust, while the visible light denotes glowing gas, and the X-rays represent very hot gas. Ordinary stars appear as blue spots with white centres, while young stars enshrouded in dust appear as red spots with white centres.

Autorska prava:

ESO/ESA/ JPL-Caltech/NASA/ D. Gouliermis (MPIA) et al.

O slici

Id:eso0834a
Tip:Opservacija
Datum objavljivanja:8. oktobar 2008.
Povezana saopštenja:eso0834
Veličina:2106 x 1989 px

O objektu

Naziv:NGC 346
Tip:Local Universe : Nebula : Type : Star Formation
Udaljenost:200000 svetlosnih godina
Constellation:Tucana
Kategorija:Nebulae

Formati slika

Veliki JPEG
1,0 MB

Wallpapers

1024x768
276,8 KB
1280x1024
416,8 KB
1600x1200
559,1 KB
1920x1200
627,6 KB
2048x1536
832,3 KB

Koordinate

Position (RA):0 59 17.90
Position (Dec):-72° 10' 47.98"
Field of view:6.99 x 6.60 arcminutes
Orijentacija:Sever je 8.3°desno od vertikale

Boje i flteri

OpsegTalasna dužinaTeleskop
X-zraci
Soft X-ray
0.00059 nmESA XMM-Newton
EPIC
Optički
V
New Technology Telescope
EFOSC2
Infracrveni
Mid-IR
8.0 μm Spitzer Space Telescope
IRAC (Spitzer)

 

Takođe pogledajte