Sub-millimetre image of a stellar cradle
Image of the giant molecular cloud G327 taken with APEX. More than 5000 spectra were taken in the J=3-2 line of the carbon monoxide molecule (CO), one of the best tracers of molecular clouds, in which star formation takes place. The bright peak in the north of the cloud is an evolved star forming region, where the gas is heated by a cluster of new stars. The most interesting region in the image is totally inconspicuous in CO: the G327 hot core, as seen in methanol contours. It is a truly exceptional source, and is one of the richest sources of emission from complex organic molecules in the Galaxy (see spectrum at bottom)
Kredit:ESO
O snímku
Id: | eso0531b |
Typ: | Koláž |
Datum zveřejnění: | 25. září 2005 |
Související články: | eso0531 |
Velikost: | 1503 x 1975 px |
O objektu
Jméno: | G327.3-0.6 |
Typ: | Milky Way : Nebula : Appearance : Dark : Molecular Cloud |
Vzdálenost: | 9500 světelné roky |
Kategorie: | Nebulae Stars |
Barvy & filtry
Pásmo | Dalekohled |
---|---|
Milimetrový Submillimetre | Atacama Pathfinder Experiment |