Composition of KBO (50000) Quaoar

Astronomy and Astrophysics

Volumn 501, Issue 1, 2009, Pages 349-357

  Morea Dalle Ore, C ^a,c   Barucci, M A ^b   Emery, J P ^d   Cruikshank, D P ^a   Dalle Ore, L V ^a   Merlin, F ^e   Alvarez Candal, A ^b   De Bergh, C ^b   Trilling, D E ^h   Perna, D ^b,f,g   Fornasier, S ^b   Mastrapa, R M E ^a,c   Dotto, E ^f  

^a NASA AMES RESEARCH CENTER   (United States)

^b OBSERVATOIRE DE PARIS   (France)

^c SETI INSTITUTE   (United States)

^d UNIVERSITY OF TENNESSEE   (United States)

^e Bldg 142   (United States)

^f INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^g UNIVERSITY OF ROME TOR VERGATA   (Italy)

^h NORTHERN ARIZONA UNIVERSITY   (United States)

Author keywords

Kuiper Belt; Techniques: Spectroscopic

Indexed keywords

CHEMICAL EVOLUTION; CRYSTALLINE FEATURE; EXCELLENT SET; HIGH RESOLUTION; KUIPER BELT; MODEL CALCULATIONS; MODEL FIT; NEAR INFRARED; NEPTUNE; ORGANIC MATERIALS; PHOTOMETRIC DATA; SIGNAL TO NOISE; SLAB MODEL; SPECTRAL MODELING; SPITZER SPACE TELESCOPE; SURFACE COMPOSITIONS; TECHNIQUES: SPECTROSCOPIC; VISIBLE AND NEAR INFRARED; WAVELENGTH RANGES;

CRYSTALLINE MATERIALS; ICE; INFRARED DEVICES; PHOTOMETRY; SPACE TELESCOPES; SPACECRAFT OBSERVATORIES; SURFACE CHEMISTRY;

SOLAR SYSTEM;

EID: 67650931810     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911752     Document Type: Article

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