| Description |
Despite of all theoretical speculations and various observationalconstraints, the nature of the dark matter in the outer Galaxy isstill unknown. Herschel/HIFI offers the unique opportunity to detector set a significant upper limit to a potential component of baryonicmatter in the form of cold gas, which is molecular in hydrogen, butdoes not form CO. Such gas can be potentially be traced through CII150 um and HF J=1-0 absorption against continuum backgroundsources. We propose a set of 7 the brightest outer Galaxy dustcontinuum sources, for which we will determine the positions of peakemission by PACS mapping. Deep integrations in CII and HF towardsthe 4 brightest peaks in these sources will potentially detect a coldgas component and will, in any case, give significant upper limits toits column density. |
| Keywords |
Herschel Space Observatory data, ESA Herschel mission dataset, far-infrared astronomy observations, submillimeter astronomy data, infrared space telescope observations, PACS photometer data, PACS spectrometer data, SPIRE photometer data, SPIRE Fourier transform spectrometer data, HIFI heterodyne spectroscopy data, far-infrared spectroscopy dataset, submillimeter spectral line observations, cold universe observations dataset, star formation infrared data, molecular cloud far-infrared observations, interstellar medium spectroscopy data, protoplanetary disk infrared observations, galaxy evolution far-infrared data, dust emission submillimeter observations, cosmic infrared background measurements, extragalactic infrared survey data, calibrated level 2 data products, FITS files astronomy, spectral cubes far-infrared, flux-calibrated maps, continuum photometry data, spectral energy distribution measurements, ESA Herschel Science Archive data |
