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Albedo and atmospheric constraints of dwarf planet Makemake from a stellar occultationORTIZ, J. L; SICARDY, B; ASSAFIN, M et al.Nature (London). 2012, Vol 491, Num 7425, pp 566-569, issn 0028-0836, 4 p.Article

Ceres ― Neither a porous nor salty ballCASTILLO-ROGEZ, Julie C.Icarus (New York, N.Y. 1962). 2011, Vol 215, Num 2, pp 599-602, issn 0019-1035, 4 p.Article

GIUSEPPE PIAZZI: THE CONTROVERSIAL DISCOVERY AND LOSS OF CERES IN 1801CUNNINGHAM, Clifford J; MARSDEN-I, Brian G; ORCHISTON, Wayne et al.Journal for the history of astronomy. 2011, Vol 42, pp 283-306, issn 0021-8286, 24 p., 3Article

A Pluto-like radius and a high albedo for the dwarf planet Eris from an occultationSICARDY, B; ORTIZ, J. L; LECACHEUX, J et al.Nature (London). 2011, Vol 478, Num 7370, pp 493-496, issn 0028-0836, 4 p.Article

HIGH-CONTRAST 3.8 μm IMAGING OF THE BROWN DWARF/PLANET-MASS COMPANION TO GJ 758CURRIE, Thayne; BAILEY, Vanessa; FABRYCKY, Daniel et al.The Astrophysical journal. 2010, Vol 721, Num 2, issn 0004-637X, L177-L181, 2Article

Tohoku-Hiroshima-Nagoya planetary spectra library: a method for characterizing planets in the visible to near infraredLUNDOCK, R; ICHIKAWA, T; OKITA, H et al.Astronomy and astrophysics (Berlin. Print). 2009, Vol 507, Num 3, pp 1649-1658, issn 0004-6361, 10 p.Article

Thermal rotational lightcurve of dwarf-planet (1) Ceres at 235 GHz with the Submillimeter ArrayMOULLET, A; GURWELL, M; CARRY, B et al.Astronomy and astrophysics (Berlin. Print). 2010, Vol 516, issn 0004-6361, L1.1-L10.4Article

ON THE METAL RICHNESS OF M DWARFS WITH PLANETSJOHNSON, John Asher; APPS, Kevin.The Astrophysical journal. 2009, Vol 699, Num 2, pp 933-937, issn 0004-637X, 5 p., 1Article

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IDENTIFYING COLLISIONAL FAMILIES IN THE KUIPER BELTMARCUS, Robert A; RAGOZZINE, Darin; MURRAY-CLAY, Ruth A et al.The Astrophysical journal. 2011, Vol 733, Num 1, issn 0004-637X, 73340.1-73340.15, 1Article

A population of Main Belt Asteroids co-orbiting with Ceres and VestaCHRISTOU, Apostolos A; WIEGERT, Paul.Icarus (New York, N.Y. 1962). 2012, Vol 217, Num 1, pp 27-42, issn 0019-1035, 16 p.Article

DISTINGUISHING CENTRAL PERTURBATIONS BY BINARY STELLAR AND PLANETARY SYSTEMS UNDER THE MODERATELY STRONG FINITE-SOURCE EFFECTCHUNG, Sun-Ju; LEE, Chung-Uk.The Astrophysical journal. 2011, Vol 741, Num 2, issn 0004-637X, 118.1-118.10, 1Article

THE DEUTERIUM-BURNING MASS LIMIT FOR BROWN DWARFS AND GIANT PLANETSSPIEGEL, David S; BURROWS, Adam; MILSOM, John A et al.The Astrophysical journal. 2011, Vol 727, Num 1, pp 766-774, issn 0004-637X, 9 p., 1Article

Structure and evolution of the first CoRoT exoplanets: probing the brown dwarf/planet overlapping mass regimeLECONTE, J; BARAFFE, I; CHABRIER, G et al.Astronomy and astrophysics (Berlin. Print). 2009, Vol 506, Num 1, pp 363-367, issn 0004-6361, 5 p.Article

Rapid planetesimal formation in turbulent circumstellar disksJOHANSEN, Anders; OISHI, Jeffrey S; MAC LOW, Mordecai-Mark et al.Nature (London). 2007, Vol 448, Num 7157, pp 1022-1025, issn 0028-0836, 4 p.Article

AN H-BAND SPECTROSCOPIC METALLICITY CALIBRATION FOR M DWARFSTERRIEN, Ryan C; MAHADEVAN, Suvrath; BENDER, Chad F et al.The Astrophysical journal. 2012, Vol 747, Num 2, issn 0004-637X, L38.1-L38.6, 2Article

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Long-term magnetic activity of a sample of M-dwarf stars from the HARPS program :I. Comparison of activity indicesGOMES DA SILVA, J; SANTOS, N. C; BONFILS, X et al.Astronomy and astrophysics (Berlin. Print). 2011, Vol 534, issn 0004-6361, A30.1-A30.17, 1Article

First-order rotation solution of an oblate rigid body under the torque of a perturber in circular orbitLARA, M; FUKUSHIMA, T; FERRER, S et al.Astronomy and astrophysics (Berlin. Print). 2010, Vol 519, issn 0004-6361, A1.1-A1.10Article

Polarimetry of the dwarf planet (136199) ErisBELSKAYA, I; BAGNULO, S; MUINONEN, K et al.Astronomy and astrophysics (Berlin. Print). 2008, Vol 479, Num 1, pp 265-269, issn 0004-6361, 5 p.Article

THE FREQUENCY OF DEBRIS DISKS AT WHITE DWARFSBARBER, Sara D; PATTERSON, Adam J; KILIC, Mukremin et al.The Astrophysical journal. 2012, Vol 760, Num 1, issn 0004-637X, 26.1-26.11, 1Article

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