CO2 synthesis in solid CO by Lyman-α photons and 200 keV protons
نویسندگان
چکیده
We have studied the synthesis of carbon dioxide from solid carbon monoxide at 16 K induced by photolysis with Lyman-α photons and by irradiation with 200 keV protons to quantitatively compare the effects of photolysis and ion irradiation on CO ice and to determine the importance of these processes in interstellar ice grains. The CO and CO2 concentrations during irradiation of an initially pure CO film evolve with fluence to a saturation value, a behaviour that is explained by a two-state model. Our results indicate that the initial CO2 production rates for both radiation processes are similar when normalized to the absorbed energy and that the solid CO2 abundance observed in the interstellar ices cannot be explained only by radiolysis and photolysis of pure solid CO.
منابع مشابه
Lyman α photolysis of solid nitromethane (CH3NO2) and D3-nitromethane (CD3NO2)--untangling the reaction mechanisms involved in the decomposition of model energetic materials.
Solid nitromethane (CH3NO2) along with its isotopically labelled counterpart D3-nitromethane (CD3NO2) ices were exposed to Lyman α photons to investigate the mechanism involved in the decomposition of energetic materials in the condensed phase. The chemical processes in the ices were monitored online and in situ via infrared spectroscopy complimented by temperature programmed desorption studies...
متن کاملOn Detecting the X–ray Silhouette of a Damped Lyman Α System
We explore the possibility of resolving an image of a damped Lyman α (DLA) system in absorption against an extended, diffuse background X–ray source. Typical columns of neutral hydrogen in DLAs are high enough to block out up to ∼ 30% of the soft X–ray flux at an observed photon energy of 0.5 keV, and we find that ∼ 1% of the area of extended X–ray sources at z & 1 have their 0.5 keV flux reduc...
متن کاملImpact polarization and charge exchange as diagnostics of proton beams
Linear polarization of the hydrogen Hα line has been observed in solar flares. This polarization is actually explained as induced by anisotropic collisional excitation of the n = 3 level by vertical proton beams with an energy of a few keV. At such energies, charge exchange between the proton beam and the local H atoms is important and must be taken into account in the statistical equilibrium e...
متن کاملStability of carbonaceous dust analogues and glycine under UV irradiation and electron bombardment.
The effect of UV photon (120-200 nm) and electron (2 keV) irradiation of analogues of interstellar carbonaceous dust and of glycine were investigated by means of IR spectroscopy. Films of hydrogenated amorphous carbon (HAC), taken as dust analogues, were found to be stable under UV photon and electron bombardment. High fluences of photons and electrons, of the order of 10(19) cm(-2), were neede...
متن کاملThe Volume Fraction of Ionized Intergalactic Gas at Redshift z = 6 . 5
The observed number density of Lyman-α sources implies a minimum volume of the inter-galactic medium that must be ionized, in order to allow the Lyman-α photons to escape attenuation. We estimate this volume by assigning to each Lyman-α emitter the minimum Stromgren sphere that would allow half its Lyman-α photons to escape. This implies a lower limit to ionized gas volume fraction of 20-50% at...
متن کامل