Star Formation in Rho Ophiuchi (original) (raw)
infrared optical X-ray
| Date: | 10.6.1994 | Time: | 3:11 UT | Exposure: | 45m |
|---|---|---|---|---|---|
| Field of View: | 15o x 15o | Emulsion: | Scotchchrome 400 | Filter: | none |
| Instrument: | f=100mm 1/2.8 | Place: | Cerro Tololo | Observer: | S. Kohle |
© Copyright by the observers
The infrared image was observed byIRAS, the X-ray image byROSATand were obtained from theSKYVIEW webpage.
In a distance of about 500 lightyears the region around Rho Ophiuchi represents the Earth's closest star nursery. Embedded in the most dense clouds of molecular gas and dust stars are born right now. The dust is emitting light in the infrared and absorbing stellar light in the optical and X-ray regime. The blue and yellow color of the nebulae in the optical image is from interstellar light reflection of embedded stars. The red emission is mainly from ionized hydrogen.
The X-ray image is a three color composit in which emission in different Rosat energy bands is represented in different colors (1/4 keV = red, 3/4 keV = green and 1.5 keV = blue). As you can easily see the dusty molecular clouds also absorb the high energy X-rays, so that these regions appear darkly red.
The IRAS image shows the thermal emission of dust at 100 microns. The dust has different temperatures and emits at wavelengths from mm to submm. Therefore there is no perfect correlation of the dust emission at 100 microns and dust absorption in the optical.
Astronomical Institutes of the University of Bonn