Sergio Pilling

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Titan, the largest satellite of Saturn, has an atmosphere chiefly made up of N(2) and CH(4) and includes traces of many simple organic compounds. This atmosphere also partly consists of haze and aerosol particles which during the last 4.5 gigayears have been processed by electric discharges, ions, and ionizing photons, being slowly deposited over the Titan(More)
In order to simulate the effects of energetic charged particles present in the solar wind colliding with the cometary gaseous formic acid molecule (HCOOH), laboratory experiments have been performed. The absolute ionisation and dissociation cross sections for this molecule interacting with solar wind particles were measured employing fast electrons in the(More)
We present experimental results obtained from photoionization and photodissociation processes of abundant interstellar CH 3-X type organic molecules like methanol (CH 3 OH), methy-lamine (CH 3 NH 2) and acetonitrile (CH 3 CN) as alternative route for the production of H + 3 in interstellar and star forming environments. The measurements were taken at the(More)
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