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| 2. |
- Gerin, M., et al.
(författare)
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Interstellar CH absorption in the diffuse interstellar medium along the sight-lines to G10.6-0.4 (W31C), W49N, and W51
- 2010
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Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 521:1, s. Article Number: L16-
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Tidskriftsartikel (refereegranskat)abstract
- We report the detection of the ground state N, J = 1, 3/2 -> 1, 1/2 doublet of the methylidyne radical CH at similar to 532 GHz and similar to 536 GHz with the Herschel/ HIFI instrument along the sight-line to the massive star-forming regions G10.6-0.4 (W31C), W49N, and W51. While the molecular cores associated with these massive star-forming regions show emission lines, clouds in the diffuse interstellar medium are detected in absorption against the strong submillimeter background. The combination of hyperfine structure with emission and absorption results in complex profiles, with overlap of the different hyperfine components. The opacities of most of the CH absorption features are linearly correlated with those of CCH, CN, and HCO+ in the same velocity intervals. In specific narrow velocity intervals, the opacities of CN and HCO+ deviate from the mean trends, giving rise to more opaque absorption features. We propose that CCH can be used as another tracer of the molecular gas in the absence of better tracers, with [CCH]/[H2] similar to 3.2 +/- 1.1 x 10-8. The observed [CN]/[CH], [CCH]/[CH] abundance ratios suggest that the bulk of the diffuse matter along the lines of sight has gas densities nH = n(H) + 2n(H2) ranging between 100 and 1000 cm-3).
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| 3. |
- Persson, Carina, 1964, et al.
(författare)
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Nitrogen hydrides in interstellar gas Herschel/HIFI observations towards G10.6-0.4 (W31C)
- 2010
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Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 521:1, s. Article Number: L45 -
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Tidskriftsartikel (refereegranskat)abstract
- The HIFI instrument on board the Herschel Space Observatory has been used to observe interstellar nitrogen hydrides along the sight-line towards G10.6-0.4 in order to improve our understanding of the interstellar chemistry of nitrogen. We report observations of absorption in NH N = 1
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| 4. |
- Kronast, F., et al.
(författare)
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Element-specific magnetic hysteresis of individual 18 nm Fe nanocubes
- 2011
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Ingår i: Nano Letters. - : American Chemical Society (ACS). - 1530-6992 .- 1530-6984. ; 11:4, s. 1710-1715
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Tidskriftsartikel (refereegranskat)abstract
- Correlating the electronic structure and magnetic response with the morphology and crystal structure of the same single ferromagnetic nanoparticle has been up to now an unresolved challenge. Here, we present measurements of the element-specific electronic structure and magnetic response as a function of magnetic field amplitude and orientation for chemically synthesized single Fe nanocubes with 18 nm edge length. Magnetic states and interactions of monomers, dimers, and trimers are analyzed by X-ray photoemission electron microscopy for different particle arrangements. The element-specific electronic structure can be probed and correlated with the changes of magnetic properties. This approach opens new possibilities for a deeper understanding of the collective response of magnetic nanohybrids in multifunctional materials and in nanomagnetic colloidal suspensions used in biomedical and engineering technologies. © 2011 American Chemical Society.
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| 5. |
- Allvin, H., et al.
(författare)
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Characteristics and Analysis of Finnish and Swedish Clinical Intensive Care Nursing Narratives
- 2010
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Ingår i: Proceedings of the NAACL HLT 2010 Second Louhi Workshop on Text and Data Mining of Health Documents. ; , s. 53 - 60
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Konferensbidrag (refereegranskat)abstract
- We present a comparative study of Finnish and Swedish free-text nursing narratives from intensive care. Although the two languages are linguistically very dissimilar, our hypothesis is that there are similarities that are important and interesting from a language technology point of view. This may have implications when building tools to support producing and using health care documentation. We perform a comparative qualitative analysis based on structure and content, as well as a comparative quantitative analysis on Finnish and Swedish Intensive Care Unit (ICU) nursing narratives. Our findings are that ICU nursing narratives in Finland and Sweden have many properties in common, but that many of these are challenging when it comes to developing language technology tools.
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| 6. |
- Durden, Chris H., et al.
(författare)
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Cost accounting and performance measurement in a just-in-time production environment
- 1999
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Ingår i: Asia Pacific Journal of Management. - : Springer. - 0217-4561 .- 1572-9958. ; 16:1, s. 111-125
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Tidskriftsartikel (refereegranskat)abstract
- There are normative statements in the literature, backed up by case observations and anecdotal evidence, which indicate that manufacturing companies operating just-in-time (JIT) production management systems should also change their cost accounting systems and place greater reliance on non-financial performance indicators. This study provides empirical evidence suggesting that JIT manufacturing companies which have made some degree of modification to their costing system demonstrate higher performance than JIT companies which have not made changes. The results also suggest that greater use of non-financial performance indicators is associated with higher performance irrespective of the production management system adopted.
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| 7. |
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| 8. |
- Hassel, Ivon, et al.
(författare)
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Towards determination of local and overall displacements of the Vasa ship structure: Effect of its mechanical connections
- 2014
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Konferensbidrag (refereegranskat)abstract
- The warship Vasa from the 17th century must be preserved for the future generations. There are many concerns currently being addressed by ongoing research efforts. The support structure is one of them, which needs to be re-designed. In order to do this, the local and overall deformation of the Ship’s structure must be identified. The earlier impregnation of PEG on the Vasa material is causing the material to creep significantly more than oak without PEG, resulting in an increasing deformation of the ship. In addition to this, the effect of the mechanical connections of the ship needs to be considered. Experimental tests were performed on a 1:1 scale replica of a representative section of the Vasa ship. Different load cases were applied in order to represent the current situation of the vessel’s connections. Linear displacement gauges as well as non-contacting image correlation systems were used as measurement methods to analyze the behaviour of the test sample. A validated computer model, using finite element method (FEM) simulations, with Vasa-material properties will be used to calculate the stiffness coefficients, which will be included in a simplified full-computer model of the entire vessel. Based on the latter, the overall and local displacements will be obtained. This is a necessary input in a full numerical model of the ship to optimize a new support structure.
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| 9. |
- Mookerjea, B., et al.
(författare)
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Chemistry of C-3 and carbon chain molecules in DR21(OH)
- 2012
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Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 546, s. Article Number: A75 (pp. 1-11)
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Tidskriftsartikel (refereegranskat)abstract
- Context. C-3 is the smallest pure carbon chain detected in the dense environment of star-forming regions, although diatomic C-2 is detected in diffuse clouds. Measurement of the abundance of C-3 and the chemistry of its formation in dense star-forming regions has remained relatively unexplored. Aims. We aim to identify the primary C-3 formation routes in dense star-forming regions following a chemical network producing species like CCH and c-C3H2 in the star-forming cores associated with DR21(OH), a high-mass star-forming region. Methods. We observed velocity resolved spectra of four ro-vibrational far-infrared transitions of C-3 between the vibrational ground state and the low-energy nu(2) bending mode at frequencies between 1654-1897 GHz using HIFI on board Herschel, in DR21(OH). Several transitions of CCH and c-C3H2 were also observed with HIFI and the IRAM 30 m telescope. Rotational temperatures and column densities for all chemical species were estimated. A gas and grain warm-up model was used to obtain estimates of densities and temperatures of the envelope. The chemical network in the model was used to identify the primary C-3 forming reactions in DR21(OH). Results. We detected C-3 in absorption in four far-infrared transitions, P(4), P(10), Q(2), and Q(4). The continuum sources MM1 and MM2 in DR21(OH), though spatially unresolved, are sufficiently separated in velocity to be identified in the C-3 spectra. All C-3 transitions are detected from the embedded source MM2 and the surrounding envelope, whereas only Q(4) and P(4) are detected toward the hot core MM1. The abundance of C-3 in the envelope and MM2 is similar to 6 x 10(-10) and similar to 3 x 10(-9), respectively. For CCH and c-C3H2, we only detect emission from the envelope and MM1. The observed CCH, C-3 and c-C3H2 abundances are most consistent with a chemical model with n(H2) similar to 5 x 10(6) cm(-3), a post-warm-up dust temperature T-max = 30 K, and a time of similar to 0.7-3 Myr. Conclusions. Post-warm-up gas phase chemistry of CH4 released from the grain at t similar to 0.2 Myr and lasting for 1 Myr can explain the observed C-3 abundance in the envelope of DR21(OH), and no mechanism involving photodestruction of PAH molecules is required. The chemistry in the envelope is similar to the warm carbon chain chemistry found in lukewarm corinos. We interpret the observed lower C-3 abundance in MM1 as compared to MM2 and the envelope to be due to the destruction of C-3 in the more evolved MM1. The timescale for the chemistry derived for the envelope is consistent with the dynamical timescale of 2 Myr derived for DR21(OH) in other studies.
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| 10. |
- Persson, Carina, 1964, et al.
(författare)
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First detection of [NII] 205 μm absorption in interstellar gas. Herschel-HIFI observations towards W31C, W49N, W51, and G34.3+0.1.
- 2014
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Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 568, s. 37-
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Tidskriftsartikel (refereegranskat)abstract
- We present high resolution [N II] 205 μm (3^P_1 − 3^P_0) spectra obtained with Herschel-HIFI towards a small sample of far-infrared bright star forming regions in the Galactic plane: All sources display an emission line profile associated directly with the H II regions themselves. For the first time we also detect absorption of the [N II] 205 μm line by extended low-density foreground material towards W 31C and W 49N over a wide range of velocities. We attribute this absorption to the warm ionised medium (WIM) and find N(N+) ≈ 1.5×10^17 cm^-2 towards both sources. This is in agreement with recent Herschel-HIFI observations of [C II] 158 μm, also observed in absorption in the same sight-lines, if ≈7–10% of all C + ions exist in the WIM on average. Using an abundance ratio of [N]/[H] = 6.76×10^-5 in the gas phase we find that the mean electron and proton volume densities are ∼0.1–0.3 cm^-3 assuming a WIM volume filling fraction of 0.1–0.4 with a corresponding line-of-sight filling fraction of 0.46–0.74. A low density and a high WIM filling fraction are also supported by RADEX modelling of the [N II] 205 μm absorption and emission together with visible emission lines attributed mainly to the WIM. The detection of the 205 μm line in absorption emphasises the importance of a high spectral resolution, and also offers a new tool for investigation of the WIM.
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