Instantaneous formation of interstellar minerals and mineral quantum dots. [PDF]
RSC AdvRoy A +13 more
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Infrared Irradiation of H<sub>2</sub>O:CO<sub>2</sub> Ice: A Combined Experimental and Computational Study of the Dissipation of CO<sub>2</sub> Vibrational Excitations. [PDF]
ACS Earth Space ChemSchrauwen JGM +5 more
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Photochemical Haze Formation on Titan and Uranus: A Comparative Review. [PDF]
Int J Mol SciDubois D.
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Infrared Multiple Photon Dissociation Spectroscopy of the H-H Stretching Mode and Low-Lying Electronic Transitions in Fe<sup>+</sup>(H<sub>2</sub>)<sub>1,2</sub> and Fe<sup>+</sup>(D<sub>2</sub>)<sub>1,2</sub>. [PDF]
J Phys Chem AJin S +4 more
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Unique Applications of para-Hydrogen Matrix Isolation to Spectroscopy and Astrochemistry. [PDF]
J Phys Chem LettWeber I, Joshi PR, Anderson DT, Lee YP.
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The origin of unidentified interstellar absorption lines
, 1939 Swings, Polydore, Öhman, Y.
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Interstellar Silicate Absorption Bands
Nature, 1970Interstellar silicate absorption is observed in the direction of the galactic centre. Most interstellar silicon seems to be in silicate form.
J A, Hackwell, R D, Gehrz, N J, Woolf
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Diffuse interstellar absorption bands
Science in China Series G: Physics, Mechanics and Astronomy, 2009The diffuse interstellar bands (DIBs) are a large number of absorption bands that are superposed on the interstellar extinction curve and are of interstellar origin. Since the discovery of the first two DIBs in the 1920s, the exact nature of DIBs still remains unclear.
FuYuan Xiang, ShunLin Liang, AiGen Li
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