Concluding remarks: Faraday Discussion on astrochemistry at high resolution.

Fifty years on from the first detailed chemical kinetic modelling of astronomical sources, I provide some introductory comments on the history of astrochemistry, summarise some personal views on the topics covered in this discussion meeting, and conclude with some thoughts on its future development. I have left out the jokes.

(Sub)stellar companions shape the winds of evolved stars.

Binary interactions dominate the evolution of massive stars, but their role is less clear for low- and intermediate-mass stars. The evolution of a spherical wind from an asymptotic giant branch (AGB) star into a nonspherical planetary nebula (PN) could be due to binary interactions. We observed a sample of AGB stars with the Atacama Large Millimeter/submillimeter Array (ALMA) and found that their winds exhibit distinct nonspherical geometries with morphological similarities to planetary nebulae (PNe). We infer that the same physics shapes both AGB winds and PNe; additionally, the morphology and AGB mass-loss rate are correlated. These characteristics can be explained by binary interaction. We propose an evolutionary scenario for AGB morphologies that is consistent with observed phenomena in AGB stars and PNe.

Complex organic molecules along the accretion flow in isolated and externally irradiated protoplanetary disks.

The birth environment of the Sun will have influenced the physical and chemical structure of the pre-solar nebula, including the attainable chemical complexity reached in the disk, important for prebiotic chemistry. The formation and distribution of complex organic molecules (COMs) in a disk around a T Tauri star is investigated for two scenarios: (i) an isolated disk, and (ii) a disk irradiated externally by a nearby massive star. The chemistry is calculated along the accretion flow from the outer disk inwards using a comprehensive network which includes gas-phase reactions, gas-grain interactions, and thermal grain-surface chemistry. Two simulations are performed, one beginning with complex ices and one with simple ices only. For the isolated disk, COMs are transported without major chemical alteration into the inner disk where they thermally desorb into the gas reaching an abundance representative of the initial assumed ice abundance. For simple ices, COMs can efficiently form on grain surfaces under the conditions in the outer disk. Gas-phase COMs are released into the molecular layer via photodesorption. For the irradiated disk, complex ices are also transported inwards; however, they undergo thermal processing caused by the warmer conditions in the irradiated disk which tends to reduce their abundance along the accretion flow. For simple ices, grain-surface chemistry cannot efficiently synthesise COMs in the outer disk because the necessary grain-surface radicals, which tend to be particularly volatile, are not sufficiently abundant on the grain surfaces. Gas-phase COMs are formed in the inner region of the irradiated disk via gas-phase chemistry induced by the desorption of strongly bound molecules such as methanol; hence, the abundances are not representative of the initial molecular abundances injected into the outer disk. These results suggest that the composition of comets formed in isolated disks may differ from those formed in externally irradiated disks with the latter composed of more simple ices.

Irradiation of water ice by C(+) ions in the cosmic environment.

We present a first-principles MD (FPMD) study of the interaction of low-energy, positively charged carbon (C(+)) projectiles with amorphous solid water clusters at 30 K. Reactions involving the carbon ion at an initial energy of 11 and 1.7 eV with a 30-molecule cluster have been investigated. Simulations indicate that the neutral isoformyl radical, COH(•), and carbon monoxide, CO, are the dominant products of these reactions. All of these reactions are accompanied by the transfer of a proton from the reacting water molecule to the ice, where it forms a hydronium ion. We find that COH(•) is formed either via a direct, "knock-out", mechanism following the impact of the C(+) projectile upon a water molecule or by creation of a COH2(+) intermediate. The direct mechanism is more prominent at higher energies. CO is generally produced following the dissociation of COH(•). More frequent production of the formyl radical, HCO(•), is observed here than in gas-phase calculations. A less commonly occurring product is the dihydroxymethyl, CH(OH)2(•), radical. Although a minor result, its existence gives an indication of the increasing chemical complexity that is possible in such heterogeneous environments.

Organic synthesis in the interstellar medium by low-energy carbon irradiation.

We present a first principles molecular dynamics (FPMD) study of the interaction of low-energy neutral carbon projectiles with amorphous solid water clusters at 30 K. Reactions involving the carbon atom at an initial energy of 11 and 1.7 eV with 30-molecule clusters have been investigated. Simulations indicate that the formation of hydroxymethylene, an intermediate in formaldehyde production, dominates at the higher energy. The reaction proceeds by fragmenting a water molecule, binding the carbon to the OH radical, and saturating the C valence with a hydrogen atom that can arise from the originally dissociated water molecule, or through a chain of proton transfer events. We identified several possible pathways for the formation of HCOH. When the initial collision occurs at the periphery of the cluster, we observe the formation of CO and the evaporation of water molecules. At the lower energy water fragmentation is not favorable, thus leading to the formation of weakly bound carbon-water complexes.

Dissociative recombination of protonated methanol.

The branching ratios of the different reaction pathways and the overall rate coefficients of the dissociative recombination reactions of CH3OH2+ and CD3OD2+ have been measured at the CRYRING storage ring located in Stockholm, Sweden. Analysis of the data yielded the result that formation of methanol or deuterated methanol accounted for only 3 and 6% of the total rate in CH3OH2+ and CD3OD2+, respectively. Dissociative recombination of both isotopomeres mainly involves fragmentation of the C-O bond, the major process being the three-body break-up forming CH3, OH and H (CD3, OD and D). The overall cross sections are best fitted by sigma = 1.2 +/- 0.1 x 10(-15) E(-1.15 +/- 0.02) cm2 and sigma = 9.6 +/- 0.9 x 10(-16) E(-1.20 +/- 0.02) cm2 for CH3OH2+ and CD3OD2+, respectively. From these values thermal reaction rate coefficients of k(T) = 8.9 +/- 0.9 x 10(-7) (T/300)(-0.59 +/- 0.02) cm3 s(-1) (CH3OH2+) and k(T) = 9.1 +/- 0.9 x 10(-7) (T/300)(-0.63 +/- 0.02) cm3 s(-1) (CD3OD2+) can be calculated. A non-negligible formation of interstellar methanol by the previously proposed mechanism via radiative association of CH3+ and H2O and subsequent dissociative recombination of the resulting CH3OH2+ ion to yield methanol and hydrogen atoms is therefore very unlikely.

Deuterated H3+ as a probe of isotope fractionation in star-forming regions.

Observations of molecular D/H ratios in the interstellar medium are used to probe the physical conditions, such as temperature, ionization fraction and the importance of gas-grain reactions. In cold, dense regions, such as cores which are collapsing to form stars, the level of deuterium fractionation depends on the conversion of H3+ into its deuterated isotopologues (H2D+, D2H+ and D3+). The relative abundances of these molecules uniquely probe the centres of these cores where other, heavier, species have frozen onto dust grains. We present models of the deuterium chemistry close to the centre of a pre-stellar core, in the last stage before the star forms, showing the dependence of the observable molecular D/H ratios on the physical parameters and rate coefficients that are assumed. We compare model predictions with the latest observations of these regions.

Insertion of tear proteins into a meibomian lipids film.

The eyelid meibomian gland secretions form the outer layer of the tear film. That layer functions as a lubricant during a blink, and as a barrier against intrusion of foreign bodies. The lipid film is also exposed to proteins present in the aqueous phase that may adsorb there, and thus form an integral part of the surface of the tear film, or possibly, cause disruption to the outermost layer. Therefore, the adsorption of tear proteins to the meibomian lipid layer was object of the present investigation. A model tear was set up coating a pendant drop of saline with a film of meibomian lipids and measuring variations of the interfacial pressure after the injection of tear proteins into the aqueous subphase at their physiological concentration. All tear proteins adsorbed at the interface causing the initial surface pressure to increase. For each protein, a limiting surface pressure at which a given protein was no longer able to insert into the lipid layer was found. Among the proteins tested, lipocalin was the most surface active one and inserted into the lipid layer in the whole range of surface pressure exerted by the meibomian lipid mixture. Lactoferrin, lysozyme and IgA also interacted with the lipids whereas albumin interacted more weakly. The timescale of the protein insertion into the lipid layer was of the order of 10(2) s. It was hypothesized that protein adsorption at the interface could be associated with structural changes. Indeed, the enzymatic activity of lysozyme was maintained in the presence of an outermost meibomian lipid layer that prevented its denaturation while exposure at the air/aqueous interface induced significant lysozime degradation. meibomian lipid composition is therefore functional to maintain tear proteins activity.

Transient and steady state focal and pattern electroretinogram nerve section losses in cats with unilateral optic.

This study shows the ketamine/xylazine anaesthetised cat is a useful model for the effect of unilateral optic nerve section on pattern electroretinograms (PERGs), especially if stimuli extending to previously untested low spatial frequencies and preferably down to the focal ERG (FERG) are included. The transient reversal rate, seldom used in animals,has advantages over steady state recording. Transient PERGs had signs of true spatial tuning, a higher amplitude and signal noise ratio and showed the effect of optic atrophy at low spatial frequencies more rapidly.

Modulation of tear film protein secretion with phosphodiesterase inhibitors.

A double-blind randomized clinical study was conducted to determine whether nicardipine hydrochloride was a useful treatment for dry eye.We examined its effect on the tear film, ocular surface and ocular comfort. Nicardipine hydrochloride, 3-isobutyl-1-methylxanthine and pilocarpine hydrochloride were dissolved in an artificial tear vehicle and applied topically to one eye of 12 subjects on separate days. Ocular physiology, ocular comfort and tear volume were assessed. The trial was repeated with nicardipine in an aqueous gel vehicle. Tears were collected and assessed for protein concentration and protein profile, using electrophoresis and mass spectrometry. Nicardipine induced conjunctival redness and symptoms of dryness and irritation. There was no change in total tear protein concentration or volume. An increase in a 68 kDa protein was observed, this was probably due to conjunctival vessel dilation and leakage of albumin. The adverse symptomatology and increased conjunctival redness experienced with nicardipine make it an undesirable treatment for dry eye.

Deuterium in the Galactic Centre as a result of recent infall of low-metallicity gas.

The Galactic Centre is the most active and heavily processed region of the Milky Way, so it can be used as a stringent test for the abundance of deuterium (a sensitive indicator of conditions in the first 1,000 seconds in the life of the Universe). As deuterium is destroyed in stellar interiors, chemical evolution models predict that its Galactic Centre abundance relative to hydrogen is D/H = 5 x 10(-12), unless there is a continuous source of deuterium from relatively primordial (low-metallicity) gas. Here we report the detection of deuterium (in the molecule DCN) in a molecular cloud only 10 parsecs from the Galactic Centre. Our data, when combined with a model of molecular abundances, indicate that D/H = (1.7 +/- 0.3) x 10(-6), five orders of magnitude larger than the predictions of evolutionary models with no continuous source of deuterium. The most probable explanation is recent infall of relatively unprocessed metal-poor gas into the Galactic Centre (at the rate inferred by Wakker). Our measured D/H is nine times less than the local interstellar value, and the lowest D/H observed in the Galaxy. We conclude that the observed Galactic Centre deuterium is cosmological, with an abundance reduced by stellar processing and mixing, and that there is no significant Galactic source of deuterium.

Multifocal, pattern and full field electroretinograms in cats with unilateral optic nerve section.

AIM: To look for a subcomponent of the mFERG generated at the optic nerve head and increasing in latency with distance from it. To compare multifocal electroretinogram (mFERG, mPERG) changes to those in full field ERGs and transient and steady state pattern and focal ERGs (PERGs, FERGs) in cats with total unilateral optic nerve section. METHOD: We recorded multifocal flash ERGs (mFERGs) at three levels of intensity and multifocal pattern ERGs (mPERGs) within 61 equal areas after total unilateral optic nerve section in five long term (> 18 month) survival cats, as part of a long term serial study of full field flash and pattern ERG changes to many stimuli, in a larger population. Cats were anaesthetised with Ketamine/Xylazine and wore Henkes electrodes with 6mm artificial pupils. Intact retinal circulation was verified by fluorescein angiography and optic nerve section by retinal photography and histology. We compared the mean and mean summed multifocal responses, from the normal and denervated eyes. We also compared the mean interocular difference around the area centralis and as a function of distance from the optic nerve head, across the horizontal meridian for the mFERG to the most intense stimulus. The degree of change was compared to that in other types of ERG, in the larger set of cats. RESULTS: mFERGs were similar across cats. Response density was flat with no prominence at the area centralis. Average summed mFERGs were similar in the normal and denervated eye. In the interocular differences a component near OP2 was reduced in the first kernel to the most intense stimulus, near OP1 and OP3 in the second kernel and locally, there was a hint of a component near OP2, which varied in latency in a ring around the disk and at the area centralis. Nevertheless, no component could be seen, varying in latency with distance from the optic nerve head, across the horizontal meridian. No mPERG was recordable in these conditions. Full field PERGs and FERGs were very reduced. Full field flash ERG amplitude changes were small (4-20%) and slower to appear than PERG changes. Degree of ERG reduction and correlation with PERG losses was greatest for the mesopic OPs, low for the scotopic tests (STR, ERG and OPs) and near zero for the mesopic ERG. The mFERG and mesopic ERG both lost OPs without overall amplitudes. CONCLUSIONS: The cat mFERG does not have a component, varying in latency with distance from the optic nerve head. The only change was qualitiatively similar to that in the light adapted ERG. With intense stimuli there were local changes around the time of OP2 near the area centralis which might be explained by local variations in ganglion cell density.

Characterization of an inwardly rectifying potassium channel in the rabbit superior lacrimal gland.

PURPOSE: To characterize the properties of an inwardly rectifying K+ (KIR) current in fresh, enzymatically isolated acinar cells from the rabbit superior lacrimal gland. METHODS: New Zealand White rabbits of both sexes were killed by injecting 45 mg/kg pentobarbital sodium, and the glands were excised. Single acinar cells were isolated enzymatically from these glands. Standard patch-clamp techniques were used to record ion currents. RESULTS: Hyperpolarizing voltages evoked KIR currents that had a conductance of 2.7 +/- 0.16 nS (n = 6) in the range -50 mV to -160 mV. The KIR current was activated with steep voltage dependence on hyperpolarization, and the conductance was approximately dependent on the square root of the external K+ concentration. Increasing the pipette Ca2+ concentration from 10(-9) M to 10(-6) M increased the conductance to 5.3 +/- 0.45 nS (n = 7). Internal substitution of K+ with various cations gave the following permeability sequence: K+ (1.0) > Rb+ (0.83) > Li+ (0.15). The KIR current was inhibited by Ba2+ (100 microns), tetraethylammonium (10 mM), and Cs+ (5 mM) but was insensitive to 4-aminopyridine (5 mM). The single-channel conductance was 43 +/- 2.7 pS (n = 11), and the relationship between between single-channel conductance (gamma) and external K+ concentration ([K]o) is given by: gamma = 7.04[K]o0.37 (pS, r2 = 0.99, P < 0.05). The relationship between [K]o and zero current potential (Erev) is given by: Erev = 35.5 log[K]o - 77.8 (mV; r2 = 0.99, P < 0.05). CONCLUSIONS: The KIR current identified in these lacrimal acini has a similar dependence on [K]o as other inward rectifiers of excitable tissues and exocrine glands. However, this study highlights that there are interspecies variations and similarities between KIR channels that could be related to their individual physiological roles. The authors' investigations suggest that one role of the KIR channel in the rabbit superior lacrimal gland acinar cells is to set and stabilize the resting membrane potential. However, this KIR channel may also be involved in secretion, as has been shown to occur in the sheep parotid gland.

Widespread choroidal insufficiency in primary open-angle glaucoma.

PURPOSE: The purpose of this study was to investigate choroidal perfusion in glaucoma, using histological and angiographic techniques. METHODS: We examined the choroidal vasculature in clinicopathological slides from 25 cases of primary open-angle glaucoma, five cases of optic atrophy, and 18 normal eyes. We measured choroidal thickness at fixed distances from the disk margin with light microscopy. Using a quantitative computer image analysis system, we established the depth of all vessels and the best fitting diameter and width-to-length ratio for each vessel in three pairs of eyes. Separate statistical analyses were done on the parapapillary area and the whole choroid. We compared standard fluorescein angiographic measures to peak choroidal filling time in a further 78 glaucoma and 84 normal eyes. RESULTS: Choroids were significantly (approximately 50 microns) thinner in glaucoma than in normal or optic atrophy irrespective of fundal position. Vessel frequency and mean diameter, relative to normal, showed greatest decrease near the choriocapillaris. Peak choroidal filling was the only fluorescein angiographic measure that was significantly delayed in glaucoma irrespective of age. CONCLUSIONS: Reduced choroidal thickness in primary open-angle glaucoma is primarily due to loss of the innermost choroidal vessels. Overall size decreases without significant flattening. These changes are not seen with optic atrophy alone and may be correlated with the delayed choroidal perfusion seen in fluorescein angiography.

Separation and characterisation of cyclic nucleotide phosphodiesterases from the lacrimal, harderian and zygomatic glands of the rabbit.

PURPOSE: To investigate the activity profile of cyclic nucleotide phosphodiesterase (PDE) isoenzymes and the effects of isoenzyme selective inhibitors in the superior and inferior lacrimal glands, Harderian gland, and zygomatic gland of the rabbit. METHODS: Protein fractions extracted from crude homogenates on an anion exchange column were examined for PDE activity using an HPLC method for detecting nucleotides. RESULTS: The superior and inferior lacrimal glands had identified PDE activity profiles. PDE I was the major type of activity and there was also a minor PDE III peak of activity. The main activity detected in the lipid secreting Harderian gland was PDE II and for the mucus secreting zygomatic gland PDE III. All glands contained PDE IV activity. The kinetics of the peak enzyme activities were examined and found similar, but not identical to the kinetics for PDE activities obtained from other tissues. Inhibitors of specific PDE classes and the general PDE inhibitor, IBMX, were tested on the peak enzyme activities. Activities designated by their substrate specificity or co-factor modification were most strongly inhibited by the corresponding class selective inhibitor. For example, PDE I activity in the lacrimal gland was most strongly inhibited by nicardipine. All activities were inhibited by IBMX. CONCLUSIONS: The superior and inferior lacrimal glands of the rabbit have the same PDE profile and this differs from the PDE subtypes detected in the mucus secreting zygomatic gland and the lipid secreting Harderian gland.

Kainic acid blocks a TTX-sensitive sodium channel in retinal horizontal cells of the turtle (Pseudemys scripta elegans).

The aim of this study was to investigate the effects of excitatory amino acids on channels found in horizontal cell membranes using patch-clamp techniques. We unexpectedly found that the excitatory amino acid receptor agonist, kainic acid, reversibly inhibited the transient tetrodotoxin (TTX)-sensitive Na+ current in isolated horizontal cell bodies and axons from the retina of the turtle (Pseudemys scripta elegans). The effect of kainic acid was antagonized by the glutamate receptor antagonist 6-cyano-7-nitroquinoxaline-2,3-dione. Kainic acid activated a non-selective cation current, a finding that was consistent with previous reports, and which would account for the kainate induced depolarisation of these cells. The inhibition of the transient TTX-sensitive Na+ current by kainic acid might be important in the modification of the kinetics of responses to excitatory amino acid analogues often observed during intracellular recording from these cells.