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dynamics. Icarus, 183:265-282.
Raymond, S.N., Quinn, T. & Lunine, J.I. (In Press). High-resolution simulations of the final assembly of Earth-like planets 2: water delivery and planetary habitability. Astrobiology Special Issue on M Stars, 7(1).
Raymond, S.N., Quinn, T. & Lunine, J.I. (2005). The formation and habitability of terrestrial planets in the presence of close-in giant planets. Icarus, 177(1):256-263.
Raymond, S.N., Quinn, T. & Lunine, J.I. (2005). Terrestrial planet formation in disks with varying surface density profiles. ApJ, 632(1, Part 1):670-676.
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Raymond, S.N., Quinn, T. & Lunine, J.I. (2005). High-resolution simulations of the final assembly of Earth-like planets 1: terrestrial accretion and dynamics: ArXiv Astrophysics e-prints.
Ivezic, Z., Juric, M., Lupton, R.H., Tabachnik, S., Quinn, T., The, S.C., Raymond, S.N., Quinn, T. & Lunine, J.I. (2005). SDSS Moving Object Catalog
Terrestrial Planet Formation in Disks with Varying Surface Density Profiles.
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Irvine, W.M. & Lunine, J.I. (2005). The Cycle of Matter in Our Galaxy: from Clouds to Comets. In: M. .C.Festou, H.U. Keller & H.A. Weaver (Eds.). Comets II (pp. 25-32). Tucson AZ: University of Arizona Press.
Raymond, S.-N., Quinn, T. & Lunine, J.-I. (2005). High Resolution Simulations of the Formation of Potentially Habitable Planets. NAI Meeting Abstracts.
Raymond, S.-N., Quinn, T. & Lunine, J.-I. (2005). Can Habitable Planets Co-exist with Hot/Warm Jupiters?. NAI Meeting Abstracts.
Raymond, S.-N., Quinn, T. & Lunine, J.-I. (2005). Terrestrial Planet Formation in Disks with Varying Surface Density Profiles.
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Lunine, J., Raymond, S. & Quinn, T. (2004). Can Habitable Terrestrial Planets Co-exist With Hot Jupiters?.
AGU Fall Meeting Abstracts [
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Email jlunine@lpl.arizona.edu Institution University of Arizona Telephone 520-621-2789 Fax 520-626-8250 Address Lunar & Planetary Lab
