The far-IR view of Sgr B2 and Orion KL
arXiv:0801.0293 · doi:10.1051/eas:0831014
Abstract
We summarize the main highlights from ISO observations towards Sgr B2 and Orion KL in the far-IR domain (~43 to 197 um). Both Star-Forming Regions are among the best sources to construct a template for more distant and unresolved regions (e.g., extragalactic). We stress some peculiarities in the interpretation (excitation and radiative transfer) of far-IR spectral lines and dust continuum emission.
''Far-Infrared and Submillimeter Emission of the Interstellar Medium: Models meet extragalactic and Galactic Observations''. Proceedings of the FIR Workshop 2007. Eds. C. Kramer, R. Simon et al
References in corpus (8)
- The far-IR spectrum of Sagittarius B2 region: Extended molecular absorption, photodissociation and photoionization
- Far-Infrared OH fluorescent emission in Sagittarius B2
- Water Vapor around Sgr B2
- A far-infrared molecular and atomic line survey of the Orion KL region
- The ISO LWS high resolution spectral survey towards Sagittarius B2
- Far-IR Excited OH Lines from Orion KL Outflows
- The Water Vapor Abundance in Orion KL Outflows
- OH rotational lines as a diagnostic of the warm neutral gas in galaxies