PAHCNP

Spectroscopy of cosmic dust analogs: study of the interaction with polycyclic aromatic hydrocarbons

 Coordinatore MAX PLANCK GESELLSCHAFT ZUR FOERDERUNG DER WISSENSCHAFTEN E.V. 

 Organization address address: Hofgartenstrasse 8
city: MUENCHEN
postcode: 80539

contact info
Titolo: Prof.
Nome: Friedrich
Cognome: Huisken
Email: send email
Telefono: +49 3641 947354
Fax: +49 3641 947308

 Nazionalità Coordinatore Germany [DE]
 Totale costo 162˙742 €
 EC contributo 162˙742 €
 Programma FP7-PEOPLE
Specific programme "People" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
 Code Call FP7-PEOPLE-2010-IEF
 Funding Scheme MC-IEF
 Anno di inizio 2011
 Periodo (anno-mese-giorno) 2011-10-01   -   2013-09-30

 Partecipanti

# participant  country  role  EC contrib. [€] 
1    MAX PLANCK GESELLSCHAFT ZUR FOERDERUNG DER WISSENSCHAFTEN E.V.

 Organization address address: Hofgartenstrasse 8
city: MUENCHEN
postcode: 80539

contact info
Titolo: Prof.
Nome: Friedrich
Cognome: Huisken
Email: send email
Telefono: +49 3641 947354
Fax: +49 3641 947308

DE (MUENCHEN) coordinator 162˙742.40

Mappa


 Word cloud

Esplora la "nuvola delle parole (Word Cloud) per avere un'idea di massima del progetto.

astronomers    dust    regions    particles    interstellar    materials    universe    laboratory    adsorption    pahs   

 Obiettivo del progetto (Objective)

'The main goal of the astrophysical laboratory-based studies is to identify and/or replicate in the laboratory the materials and processes which occur in the universe. The materials on the scope of this project are the polycyclic aromatic hydrocarbons (PAHs) and the particles which constitute the cosmic dust. Both of them are present in a number of regions of space and – according to recent results – are simultaneously formed during the condensation processes from the gas phase in circumstellar environments. Therefore, the adsorption of the PAHs by the dust particles must occur in those regions. The aim of this project is to study the changes induced on the PAHs by the adsorption on the dust analogs in the laboratory, with two main objectives; 1) characterization of the spectroscopic changes upon adsorption, and 2) studying the evolution of the PAHs adsorbed under UV radiation and temperature changes. Ultimately, these studies will provide the astronomers with the necessary information to positively identify these species in the interstellar medium.'

Introduzione (Teaser)

In the past, interstellar dust was an annoyance because it obscures objects astronomers want to observe. A new look at the dust permeating the Universe provided them with ways to identify organic matter created naturally by stars.

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