142 BIBLIOGRAPHY tel-00785991, version 1 - 7 Feb 2013 Binzel, R. P., Morbidelli, A., Merouane, S., DeMeo, F. E., Birlan, M., Vernazza, P., Thomas, C. A., Rivkin, A. S., Bus, S. J., & Tokunaga, A. T. 2010. Earth encounters as the origin of fresh surfaces on near-Earth asteroids. Nature, 463(Jan.), 331–334. Birlan, M., & Nedelcu, A. 2010 (Mar.). The Physics of Asteroids and Their Junction with Dynamics. Pages 229–250 of: Souchay, J., & Dvorak, R. (eds), Lecture notes in physics, berlin springer verlag. Lecture Notes in Physics, Berlin Springer Verlag, vol. 790. Birlan, M., & Popescu, M. 2011 (Oct.). Modelling asteroid spectra: few examples. Page 810 of: Epsc-dps joint meeting 2011. Birlan, M., Barucci, M. A., & Fulchignoni, M. 1996a. G-mode analysis of the reflection spectra of 84 asteroids. A&A, 305(Jan.), 984–+. Birlan, M., Barucci, M. A., Angeli, C. A., Doressoundiram, A., & de Sanctis, M. C. 1996b. Rotational properties of asteroids: CCD observations of nine small asteroids. Planet. Space Sci., 44(June), 555–558. Birlan, M., Barucci, M. A., Vernazza, P., Fulchignoni, M., Binzel, R. P., Bus, S. J., Belskaya, I., & Fornasier, S. 2004a. Near-IR spectroscopy of asteroids 21 Lutetia, 89 Julia, 140 Siwa, 2181 Fogelin and 5480 (1989YK8), potential targets for the Rosetta mission; remote observations campaign on IRTF. New astronomy, 9(June), 343–351. Birlan, M., Barucci, A., & Thuillot, W. 2004b. Solar system observations by remote observing technique: useful experience for robotic telescope strategies. Astronomische nachrichten, 325(Oct.), 571–573. Birlan, M., Vernazza, P., Fulchignoni, M., Barucci, M. A., Descamps, P., Binzel, R. P., & Bus, S. J. 2006. Near infra-red spectroscopy of the asteroid 21 Lutetia. I. New results of long-term campaign. A&A, 454(Aug.), 677–681. Birlan, M., Binzel, R. P., Nedelcu, D., Vernazza, P., Barucci, A., Gasc, S., Fulchignoni, M., & Dotto, E. 2009 (Sept.). Physical Characterization of Asteroids Candidates of Marco Polo Mission. Pages 34.08–+ of: Aas/division for planetary sciences meeting abstracts 41. AAS/- Division for Planetary Sciences Meeting Abstracts, vol. 41. Birlan, M., Nedelcu, D. A., Descamps, P., Berthier, J., Marchis, F., Merouane, S., & Popescu, M. 2011. Spectral properties of (854) Frostia, (1333) Cevenola and (3623) Chaplin. MNRAS, 415(July), 587–595. Birlan, M., Popescu, M., Vernazza, P., Nedelcu, D. A., & Groussin, O. 2012. Spectroscopy of Aasteroid Pairs. Lpi contributions, 1667(May), 6098. Boattini, A., D’Abramo, G., Scholl, H., Hainaut, O. R., Boehnhardt, H., West, R., Carpino, M., Hahn, G., Michelsen, R., Forti, G., Pravec, P., Valsecchi, G. B., & Asher, D. J. 2004. Near Earth Asteroid search and follow-up beyond 22nd magnitude. A pilot program with ESO telescopes. A&A, 418(May), 743–750. Britt, D. T., Tholen, D. J., Bell, J. F., & Pieters, C. M. 1992. Comparison of asteroid and meteorite spectra - Classification by principal component analysis. Icarus, 99(Sept.), 153– 166. Brunetto, R., & Strazzulla, G. 2005. Elastic collisions in ion irradiation experiments: A mechanism for space weathering of silicates. Icarus, 179(Dec.), 265–273.
BIBLIOGRAPHY 143 Brunetto, R., Vernazza, P., Marchi, S., Birlan, M., Fulchignoni, M., Orofino, V., & Strazzulla, G. 2006. Modeling asteroid surfaces from observations and irradiation experiments: The case of 832 Karin. Icarus, 184(Oct.), 327–337. Burbine, T. H., Buchanan, P. C., Dolkar, T., & Binzel, R. P. 2009. Pyroxene mineralogies of near-Earth vestoids. Meteoritics and planetary science, 44(Oct.), 1331–1341. Bus, S. J., & Binzel, R. P. 2002a. Phase II of the Small Main-Belt Asteroid Spectroscopic SurveyA Feature-Based Taxonomy. Icarus, 158(July), 146–177. Bus, S. J., & Binzel, R. P. 2002b. Phase II of the Small Main-Belt Asteroid Spectroscopic SurveyThe Observations. Icarus, 158(July), 106–145. tel-00785991, version 1 - 7 Feb 2013 Bus, S. J., Denault, A. J., Rayner, J. T., Binzel, R. P., & Birlan, M. 2002 (Nov.). Remote observing at the NASA Infrared Telescope Facility (IRTF). Pages 94–99 of: Kibrick, R. I. (ed), Society of photo-optical instrumentation engineers (spie) conference series. Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, vol. 4845. Carruba, V., Michtchenko, T. A., Roig, F., Ferraz-Mello, S., & Nesvorný, D. 2005. On the V-type asteroids outside the Vesta family. I. Interplay of nonlinear secular resonances and the Yarkovsky effect: the cases of 956 Elisa and 809 Lundia. A&A, 441(Oct.), 819–829. Cellino, A., Pannunzio, R., Zappala, V., Farinella, P., & Paolicchi, P. 1985. Do we observe light curves of binary asteroids? A&A, 144(Mar.), 355–362. Chapman, C. R. 1996. S-Type Asteroids, Ordinary Chondrites, and Space Weathering: The Evidence from Galileo’s Fly-bys of Gaspra and Ida. Meteoritics and planetary science, 31(Oct.), 699–725. Chapman, C. R. 2004. Space Weathering of Asteroid Surfaces. Annual review of earth and planetary sciences, 32(May), 539–567. Chapman, C. R., Johnson, T. V., & McCord, T. B. 1971. A Review of Spectrophotometric Studies of Asteroids. Nasa special publication, 267, 51. Clark, B. E., Veverka, J., Helfenstein, P., Thomas, P. C., Bell, J. F., Harch, A., Robinson, M. S., Murchie, S. L., McFadden, L. A., & Chapman, C. R. 1999. NEAR Photometry of Asteroid 253 Mathilde. Icarus, 140(July), 53–65. Clark, B. E., Hapke, B., Pieters, C., & Britt, D. 2002. Asteroid Space Weathering and Regolith Evolution. Asteroids iii, 585–599. Cloutis, E. A., & Gaffey, M. J. 1991. Pyroxene spectroscopy revisited - Spectral-compositional correlations and relationship to geothermometry. J. Geophys. Res., 96(Dec.), 22809. Cloutis, E. A., Gaffey, M. J., Jackowski, T. L., & Reed, K. L. 1986a. Calibrations of phase abundance, composition, and particle size distribution for olivine-orthopyroxene mixtures from reflectance spectra. J. Geophys. Res., 91, 641–653. Cloutis, E. A., Gaffey, M. J., Jackowski, T. L., & Reed, K. L. 1986b. Calibrations of phase abundance, composition, and particle size distribution for olivine-orthopyroxene mixtures from reflectance spectra. J. Geophys. Res., 91(Oct.), 11641.
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