First detection of hydrogen isocyanide (HNC) in Titan's atmosphere

Astronomy and Astrophysics

Volumn 536, Issue , 2011, Pages

  Moreno, R ^a   Lellouch, E ^a   Lara, L M ^b   Courtin, R ^a   Bockelee Morvan D ^a   Hartogh, P ^c   Rengel, M ^c   Biver, N ^a   Banaszkiewicz, M ^d   Gonzalez A ^b,c  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^c MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^d Borowiec Astrogeodynamic Observatory   (Poland)

Author keywords

Planets and satellites: individual: Titan; Submillimeter: planetary systems; Techniques: spectroscopic

Indexed keywords

COLUMN DENSITY; DISSOCIATIVE RECOMBINATIONS; EMISSION LINES; HERSCHEL SPACE OBSERVATORIES; ISOCYANIDES; NEUTRAL ATMOSPHERE; PLANETS AND SATELLITES: INDIVIDUAL: TITAN; RADIATIVE TRANSFER MODELING; ROTATIONAL TRANSITION; SUBMILLIMETER: PLANETARY SYSTEMS; TECHNIQUES: SPECTROSCOPIC; TITAN'S ATMOSPHERE; VERTICAL PROFILE;

ASTRONOMY; DISSOCIATION; HYDROGEN; SATELLITES;

CYANIDES;

EID: 83755196054     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201118189     Document Type: Article

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