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  • Cloutis, E. A.; Binzel, R. P.; McCoy, Timothy J. (2006)
  • Ferreira, J. F.; Tanga, P.; Spoto, Federica; Machado, P.; Herald, D. (2022)
    Context. The technique of stellar occultations, greatly enhanced by the publication of the Gaia data releases, permits not only the determination of asteroid size and shape, but also the retrieval of additional, very ...
  • Su, Kate Y. L.; Rieke, George H.; Malhotra, Renu; Stapelfeldt, Karl R.; Hughes, A. M.; Bonsor, Amy; Wilner, David J.; Balog, Zoltan; Watson, Dan M.; Werner, Michael W.; Misselt, Karl A. (2013)
    Vega and Fomalhaut are similar in terms of mass, ages, and global debris disk properties; therefore, they are often referred to as "debris disk twins." We present Spitzer 10-35 µm spectroscopic data centered at ...
  • Collin, Rachel; Venera-Pontón, Dagoberto E. (The Smithsonian Institution, 2020)
    This is the fasta file of the COI sequences used to generate Figure 1 and used the the 2020 Invertebrate Biology paper: <B>How I wonder what you are: Can DNA barcoding identify the larval asteroids of Panama?</B>
  • McCoy, Timothy J.; Mittlefehldt, D. W.; Wilson, L. (Univ. of Arizona Press, 2006)
  • Taylor, G. J.; Keil, Klaus; McCoy, Timothy J.; Haack, Henning; Scott, Edward R. D. (1993)
  • Novakovic, Bojan; Vokrouhlický, David; Spoto, Federica; Nesvorný, David (2022)
    Collisions are one of the key processes shaping planetary systems. Asteroid families are outcomes of such collision still identifiable across our solar system. The families provide a unique view of catastrophic disruption ...
  • Pravec, P.; Fatka, P.; Vokrouhlicky, D.; Scheirich, P.; Durech, J.; Scheeres, D. J.; Kusnirak, P.; Hornoch, K.; Galad, A.; Pray, D. P.; Krugly, Yu N.; Burkhonovg, O.; Ehgamberdiev, Sh A.; Pollockh, J.; Moskovitz, N.; Thirouin, A.; Ortiz, J. L.; Morales, N.; Husarik, M.; Inasaridze, R. Ya; Oey, J.; Polishook, D.; Hanus, J.; Kucakova, H.; Vratil, J.; Vilagi, J.; Gajdos, S.; Kornos, L.; Veres, P.; Gaftonyuk, N. M.; Hromakina, T.; Sergeyev, V.; Slyusarev, I. G.; Ayvazian, V. R.; Cooney, W. R.; Gross, J.; Terrell, D.; Colas, F.; Vachier, F.; Slivan, S.; Skiff, B.; Marchis, F.; Ergashev, K. E.; Kim, D-H; Aznarz, A.; Serra-Ricart, M.; Behrend, R.; Roy, R.; Manzini, F.; Molotova, I. E. (2019)
    We studied a sample of 93 asteroid pairs, i.e., pairs of genetically related asteroids that are on highly similar heliocentric orbits. We estimated times elapsed since separation of pair members (i.e., pair age) that are ...
  • Ludwig, Hubert (Museum of Comparative Zoology, 1905)
  • Downey, Maureen E. (Smithsonian Institution Press, 1975)
  • Libourel, Guy; Corrigan, Catherine M. (2014)
    At present, we know of ~600,000 asteroids in the asteroid belt, and there are very likely millions more. Orbiting the Sun between Mars and Jupiter, they are thought to be the shattered remnants of small bodies formed within ...
  • Chaplin, W. J.; Sanchis-Ojeda, R.; Campante, T. L.; Handberg, R.; Stello, D.; Winn, J. N.; Basu, S.; Christensen-Dalsgaard, J.; Davies, G. R.; Metcalfe, T. S.; Buchhave, L. A.; Fischer, D. A.; Bedding, T. R.; Cochran, W. D.; Elsworth, Y.; Gilliland, R. L.; Hekker, S.; Huber, D.; Isaacson, H.; Karoff, C.; Kawaler, S. D.; Kjeldsen, H.; Latham, D. W.; Lund, M. N.; Lundkvist, M.; Marcy, G. W.; Miglio, A.; Barclay, T.; Lissauer, J. J. (2013)
    Results on the obliquity of exoplanet host stars the angle between the stellar spin axis and the planetary orbital axis provide important diagnostic information for theories describing planetary formation. Here we present ...
  • Mombarg, Joey S. G.; Dotter, Aaron; Van Reeth, Timothy; Tkachenko, Andrew; Gebruers, Sarah; Aerts, Conny (2020)
    It has been known for several decades that transport of chemical elements is induced by the process of microscopic atomic diffusion. Yet the effect of atomic diffusion, including radiative levitation, has hardly been studied ...
  • Chaplin, W. J.; Appourchaux, T.; Elsworth, Y.; García, R. A.; Houdek, G.; Karoff, C.; Metcalfe, T. S.; Molenda-Zakowicz, J.; Monteiro, M. J. P. F. G.; Thompson, M. J.; Brown, T. M.; Christensen-Dalsgaard, J.; Gilliland, R. L.; Kjeldsen, H.; Borucki, William J.; Koch, D.; Jenkins, J. M.; Ballot, J.; Basu, S.; Bazot, M.; Bedding, T. R.; Benomar, O.; Bonanno, A.; Brandão, I. M.; Bruntt, H.; Campante, T. L.; Creevey, O. L.; Di Mauro, M. P.; Dogan, G.; Dreizler, S.; Eggenberger, P.; Esch, L.; Fletcher, S. T.; Frandsen, S.; Gai, N.; Gaulme, P.; Handberg, R.; Hekker, S.; Howe, R.; Huber, D.; Korzennik, S. G.; Lebrun, J. C.; Leccia, S.; Martic, M.; Mathur, S.; Mosser, B.; New, R.; Quirion, P. O.; Régulo, C.; Roxburgh, I. W.; Salabert, D.; Schou, J.; Sousa, S. G.; Stello, D.; Verner, G. A.; Arentoft, T.; Barban, C.; Belkacem, K.; Benatti, S.; Biazzo, K.; Boumier, P.; Bradley, P. A.; Broomhall, A. M.; Buzasi, D. L.; Claudi, R. U.; Cunha, M. S.; D'Antona, F.; Deheuvels, S.; Derekas, A.; García Hernández, A.; Giampapa, M. S.; Goupil, M. J.; Gruberbauer, M.; Guzik, J. A.; Hale, S. J.; Ireland, M. J.; Kiss, L. L.; Kitiashvili, I. N.; Kolenberg, K.; Korhonen, H.; Kosovichev, A. G.; Kupka, F.; Lebreton, Y.; Leroy, B.; Ludwig, H. G.; Mathis, S.; Michel, E.; Miglio, A.; Montalbán, J.; Moya, A.; Noels, A.; Noyes, R. W.; Pallé, P. L.; Piau, L.; Preston, H. L.; Roca Cortés, T.; Roth, M.; Sato, K. H.; Schmitt, J.; Serenelli, A. M.; Silva Aguirre, V.; Stevens, I. R.; Suárez, J. C.; Suran, M. D.; Trampedach, R.; Turck-Chièze, S.; Uytterhoeven, K.; Ventura, R.; Wilson, P. A. (2010)
    We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5 days of science operations, reveal high signal-to-noise solar-like oscillation ...

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