Radiolysis of H2O:CO2 ices by heavy energetic cosmic ray analogs

Astronomy and Astrophysics

Volumn 523, Issue 5, 2010, Pages

  Pilling, S ^a   Seperuelo Duarte, E ^b   Domaracka, A ^c   Rothard, H ^c   Boduch, P ^c   Da Silveira, E F ^d  

^a INSTITUTO DE PESQUISA E DESENVOLVIMENTO   (Brazil)

^b CEFET   (Brazil)

^c UNIVERSITÉ DE CAEN   (France)

^d PONTIFICAL CATHOLIC UNIVERSITY OF RIO DE JANEIRO   (Brazil)

Author keywords

astrochemistry; cosmic rays; ISM: molecules; molecular data; planets and satellites: composition; solar wind

Indexed keywords

ASTROCHEMISTRY; ASTROPHYSICAL ICE ANALOGS; C-SI SUBSTRATES; COLUMN DENSITY; DISSOCIATION CROSS SECTIONS; ENERGETIC ION; EXPERIMENTAL STUDIES; FLUENCES; FOURIER TRANSFORM INFRARED SPECTROMETER; GAS SAMPLES; HEAVY-ION ACCELERATOR; IN-SITU ANALYSIS; ISM: MOLECULES; MIXED H; MOLECULAR CLOUDS; MOLECULAR DATA; PHYSICOCHEMICAL INTERACTIONS; PLANETS AND SATELLITES: COMPOSITION; RELATIVE ABUNDANCE; SPUTTERING YIELDS;

ASTROPHYSICS; CLOUDS; COSMIC RAYS; COSMOLOGY; FOURIER TRANSFORMS; LINEAR ACCELERATORS; PETROLEUM TAR; PLANETS; RADIATION CHEMISTRY; RADIOLYSIS; SATELLITES; SOLAR WIND; SPUTTERING;

IONS;

EID: 78549257432     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015123     Document Type: Article

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