イソシアン化水素
出典: フリー百科事典『ウィキペディア（Wikipedia）』 (2020/01/31 18:09 UTC 版)
イソシアン化水素（イソシアンかすいそ、hydrogen isocyanide）は、分子式HNCで表される化合物である。シアン化水素 (HCN) の互変異性体である。星間物質として遍在し、宇宙化学の分野では重要な化合物の1つである。
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- ^ The suffix ylidyne refers to the loss of three hydrogen atoms from the nitrogen atom in azanium (NH+
4) See the IUPAC Red Book 2005 Table III, "Suffixes and endings", p. 257. - ^ Pau, Chin Fong; Hehre, Warren J. (1982-02-01). “Heat of formation of hydrogen isocyanide by ion cyclotron double resonance spectroscopy”. The Journal of Physical Chemistry 86 (3): 321-322. doi:10.1021/j100392a006. ISSN 0022-3654.
- ^ a b c Tennekes, P. P. (2006). “HCN and HNC mapping of the protostellar core Chamaeleon-MMS1”. Astronomy and Astrophysics 456 (3): 1037-1043. arXiv:astro-ph/0606547. Bibcode: 2006A&A...456.1037T. doi:10.1051/0004-6361:20040294.
- ^ Hirota, T. (1998). “Abundances of HCN and HNC in Dark Cloud Cores”. Astrophysical Journal 503 (2): 717-728. Bibcode: 1998ApJ...503..717H. doi:10.1086/306032.
- ^ a b Bentley, J. A. (1993). “Highly virationally excited HCN/HNC: Eigenvalues, wave functions, and stimulated emission pumping spectra”. J. Chem. Phys. 98 (7): 5209. Bibcode: 1993JChPh..98.5207B. doi:10.1063/1.464921.
- ^ a b Schilke, P. (1992). “A study of HCN, HNC and their isotopomers in OMC-1. I. Abundances and chemistry”. Astronomy and Astrophysics 256: 595-612. Bibcode: 1992A&A...256..595S.
- ^ a b Pratap, P. (1997). “A Study of the Physics and Chemistry of TMC-1”. Astrophysical Journal 486 (2): 862-885. Bibcode: 1997ApJ...486..862P. doi:10.1086/304553.
- ^ Loenen, A. F. (2007). “Molecular properties of (U)LIRGs: CO, HCN, HNC and HCO+”. Proceedings IAU Symposium 242: 1-5.
- ^ Skurski, P. (2001). “Ab initio electronic structure of HCN- and HNC- dipole-bound anions and a description of electron loss upon tautomerization”. J. Chem. Phys. 114 (17): 7446. Bibcode: 2001JChPh.114.7443S. doi:10.1063/1.1358863.
- ^ Jakubetz, W.; Lan, B. L. (1997). “A simulation of ultrafast state-selective IR-laser-controlled isomerization of hydrogen cyanide based on global 3D ab initio potential and dipole surfaces”. Chem. Phys. 217 (2-3): 375-388. Bibcode: 1997CP....217..375J. doi:10.1016/S0301-0104(97)00056-6.
- ^ a b Turner, B. E. (1997). “The Physics and Chemistry of Small Translucent Molecular Clouds. VIII. HCN and HNC”. Astrophysical Journal 483 (1): 235-261. Bibcode: 1997ApJ...483..235T. doi:10.1086/304228.
- ^ a b Hiraoka, K. (2006). “How are CH3OH, HNC/HCN, and NH3 Formed in the Interstellar Medium?”. AIP Conf. Proc. 855: 86-99. doi:10.1063/1.2359543.
- ^ Doty, S. D. (2004). “Physical-chemical modeling of the low-mass protostar IRAS 16293-2422”. Astronomy and Astrophysics 418 (3): 1021-1034. arXiv:astro-ph/0402610. Bibcode: 2004A&A...418.1021D. doi:10.1051/0004-6361:20034476.
- ^ “The UMIST Database for Astrochemistry”. 2019年2月27日閲覧。
- ^ Millar, T. J. (1997). “The UMIST database for astrochemistry 1995”. Astronomy and Astrophysics Supplement Series 121: 139-185. arXiv:1212.6362. Bibcode: 1997A&AS..121..139M. doi:10.1051/aas:1997118.
- ^ Snyder, L. E.; Buhl, D. (1971). “Observations of Radio Emission from Interstellar Hydrogen Cyanide”. Astrophysical Journal 163: L47-L52. Bibcode: 1971ApJ...163L..47S. doi:10.1086/180664.
- ^ Henkel, C. (1988). “Molecules in external galaxies: the detection of CN, C2H, and HNC, and the tentative detection of HC3N”. Astronomy and Astrophysics 201: L23-L26. Bibcode: 1988A&A...201L..23H.
- ^ Irvine, W. M., et al. (1996) "Spectroscopic evidence for interstellar ices in comet Hyakutake." 03 October 1996, Nature, 383, 418‒420.
- ^ 菅原春菜、「彗星の有機分子とその物質進化への役割」 『地球化学』 2016年 50巻 2号 p.77-96, doi:10.14934/chikyukagaku.50.77
- ^ Goldsmith, P. F. (1986). “Variations in the HCN/HNC Abundance Ratio in the Orion Molecular Cloud”. Astrophysical Journal 310: 383-391. Bibcode: 1986ApJ...310..383G. doi:10.1086/164692.
- ^ Helmich, F. P.; van Dishoeck, E. F. (1997). “Physical and chemical variations within the W3 star-forming region”. Astronomy and Astrophysics 124 (2): 205-253. Bibcode: 1997A&AS..124..205H. doi:10.1051/aas:1997357.
- ^ Zubritsky, Elizabeth (2014年8月11日). “RELEASE 14-038 - NASA's 3-D Study of Comets Reveals Chemical Factory at Work”. NASA. 2014年8月12日閲覧。
- ^ Cordiner, M.A. (11 August 2014). “Mapping the Release of Volatiles in the Inner Comae of Comets C/2012 F6 (Lemmon) and C/2012 S1 (ISON) Using the Atacama Large Millimeter/Submillimeter Array”. The Astrophysical Journal 792 (1): L2. arXiv:1408.2458. Bibcode: 2014ApJ...792L...2C. doi:10.1088/2041-8205/792/1/L2 2014年8月12日閲覧。.
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