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)
Źródło:ESO
O zdjęciu
Identyfikator: | eso0531b |
Typ: | Kolaż |
Data publikacji: | 25 września 2005 |
Powiązane komunikaty: | eso0531 |
Rozmiar: | 1503 x 1975 px |
O obiekcie
Nazwa: | G327.3-0.6 |
Typ: | Milky Way : Nebula : Appearance : Dark : Molecular Cloud |
Odległość: | 9500 lat świetlnych |
Kategoria: | Nebulae Stars |
Kolory i filtry
Pasmo | Teleskop |
---|---|
Milimetrowy Submillimetre | Atacama Pathfinder Experiment |