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- Decin, L., et al.
(författare)
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Silicon in the dust formation zone of IRC+10216
- 2010
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Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 518, s. L143-
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Tidskriftsartikel (refereegranskat)abstract
- The interstellar medium is enriched primarily by matter ejected from evolved low and intermediate mass stars. The outflows from these stars create a circumstellar envelope in which a rich gas-phase and dust-nucleation chemistry takes place. We observed the nearest carbon-rich evolved star, IRC + 10216, using the PACS (55-210 mu m) and SPIRE (194-672 mu m) spectrometers on board Herschel. We find several tens of lines from SiS and SiO, including lines from the v = 1 vibrational level. For SiS these transitions range up to J = 124-123, corresponding to energies around 6700 K, while the highest detectable transition is J = 90-89 for SiO, which corresponds to an energy around 8400 K. Both species trace the dust formation zone of IRC + 10216, and the broad energy ranges involved in their detected transitions permit us to derive the physical properties of the gas and the particular zone in which each species has been formed. This allows us to check the accuracy of chemical thermodynamical equilibrium models and the suggested depletion of SiS and SiO due to accretion onto dust grains.
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| 2. |
- López, A., et al.
(författare)
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Laboratory characterization and astrophysical detection of vibrationally excited states of vinyl cyanide in Orion-KL
- 2014
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Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 572
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Tidskriftsartikel (refereegranskat)abstract
- Context. We perform a laboratory characterization in the 18–1893 GHz range and astronomical detection between 80–280 GHz in Orion-KL with IRAM-30 m of CH2CHCN (vinyl cyanide) in its ground and vibrationally excited states. Aims. Our aim is to improve the understanding of rotational spectra of vibrationally excited vinyl cyanide with new laboratory data and analysis. The laboratory results allow searching for these excited state transitions in the Orion-KL line survey. Furthermore, rotational lines of CH2CHCN contribute to the understanding of the physical and chemical properties of the cloud. Methods. Laboratory measurements of CH2CHCN made on several different frequency-modulated spectrometers were combined into a single broadband 50–1900 GHz spectrum and its assignment was confirmed by Stark modulation spectra recorded in the 18–40 GHz region and by ab-initio anharmonic force field calculations. For analyzing the emission lines of vinyl cyanide detected in Orion-KL we used the excitation and radiative transfer code (MADEX) at LTE conditions. Results. Detailed characterization of laboratory spectra of CH2CHCN in nine different excited vibrational states: ?11 = 1, ?15 = 1, 2) ⇔ (?10 = 1,?15 = 1) ⇔ (?11 = 1,?14 = 1), and ?11 = 4 are determined, as well as the detection of transitions in the ?11 = 2and ?11 = 2, ?10 = 1 ⇔ (?11 = 1,?15 = 1), ?11 = 3/?15 = 2/?14 = 1, (?11 = 1,?10 = 1) ⇔ (?11 = 2,?15 = 1), ?9 = 1, (?11 = 1,?15 = The rotational transitions of the ground state of this molecule emerge from four cloud components of hot core nature, which trace the ?11 = 3 states for the first time in Orion-KL and of those in the ?10 = 1 ⇔ (?11 = 1,?15 = 1) dyad of states for the first time in space. physical and chemical conditions of high mass star forming regions in the Orion-KL Nebula. The lowest energy vibrationally excited states of vinyl cyanide, such as ?11 = 1 (at 328.5 K), ?15 = 1 (at 478.6 K), ?11 = 2 (at 657.8 K), the ?10 = 1 ⇔ (?11 = 1,?15 = 1) dyad (at 806.4/809.9 K), and ?11 = 3 (at 987.9 K), are populated under warm and dense conditions, so they probe the hottest parts of the Orion-KL source. The vibrational temperatures derived for the ?11 = 1, ?11 = 2, and ?15 = 1 states are 252 ± 76K, 242 ± 121K, column density of CH2CHCN in the ground state is (3.0 ± 0.9) × 1015 cm−2. We report the detection of methyl isocyanide (CH3NC) and 227 ± 68K, respectively; all of them are close to the mean kinetic temperature of the hot core component (210K). The total for the first time in Orion-KL and a tentative detection of vinyl isocyanide (CH2CHNC). We also give column density ratios between the cyanide and isocyanide isomers, obtaining a N(CH3NC)/N(CH3CN) ratio of 0.002. Conclusions. Laboratory characterization of many previously unassigned vibrationally excited states of vinyl cyanide ranging from microwave to THz frequencies allowed us to detect these molecular species in Orion-KL. Column density, rotational and vibrational temperatures for CH2CHCN in their ground and excited states, and the isotopologues have been constrained by means of a sample of more than 1000 lines in this survey.
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