Extreme collisions between planetesimals as the origin of warm dust around a Sun-like star

[1]  A. Tsuchiyama,et al.  Compositional dependence of infrared absorption spectra of crystalline silicates - III. Melilite solid solution , 2007 .

[2]  Prospects for detection of catastrophic collisions in debris disks , 2005, astro-ph/0503551.

[3]  David E. Trilling,et al.  Decay of Planetary Debris Disks , 2005 .

[4]  Thomas L. Hayward,et al.  Mid-infrared images of beta Pictoris and the possible role of planetesimal collisions in the central disk. , 2005, Nature.

[5]  M. Min,et al.  The building blocks of planets within the ‘terrestrial’ region of protoplanetary disks , 2004, Nature.

[6]  Ben Zuckerman,et al.  Young Stars Near the Sun , 2004 .

[7]  M. Hanner,et al.  3-14 Micron Spectroscopy of Comets C/2002 O4 (Hönig), C/2002 V1 (NEAT), C/2002 X5 (Kudo-Fujikawa), C/2002 Y1 (Juels-Holvorcem), and 69P/Taylor and the Relationships among Grain Temperature, Silicate Band Strength, and Structure among Comet Families , 2004, astro-ph/0404360.

[8]  S. Kenyon,et al.  Detecting the Dusty Debris of Terrestrial Planet Formation , 2004, astro-ph/0401343.

[9]  B. Zuckerman,et al.  Dusty Debris Disks as Signposts of Planets: Implications for Spitzer Space Telescope , 2003, astro-ph/0311546.

[10]  G. Tagliaferri,et al.  Fast-rotating Nearby Solar-type Stars , 2003 .

[11]  Harold F. Levison,et al.  Recent Origin of the Solar System Dust Bands , 2003 .

[12]  Wm. A. Wheaton,et al.  2MASS All Sky Catalog of point sources. , 2003 .

[13]  A. Tsuchiyama,et al.  Compositional dependence of infrared absorption spectra of crystalline silicate: II. Natural and synthetic olivines , 2003 .

[14]  G. Tagliaferri,et al.  Fast-rotating nearby solar-type stars - II. Li abundances, ¿ sin i and X-ray luminosities relationships , 2003 .

[15]  R. Laureijs,et al.  A 25 micron search for Vega-like disks around main-sequence stars with ISO , 2002 .

[16]  C. Chen,et al.  A Possible Massive Asteroid Belt around ζ Leporis , 2001, astro-ph/0109216.

[17]  B. Zuckerman.  Dusty Circumstellar Disks , 2001 .

[18]  Elizabeth A. Lada,et al.  Disk Frequencies and Lifetimes in Young Clusters , 2001, astro-ph/0104347.

[19]  B. Draine,et al.  Infrared Emission from Interstellar Dust Ii. the Diffuse Interstellar Medium , 2000 .

[20]  Z. Sekanina,et al.  Thermal Infrared Imaging and Spectroscopy of Comet Hale-Bopp (C/1995 O1) , 2000 .

[21]  J. Nuth,et al.  Evolving Optical Properties of Annealing Silicate Grains: From Amorphous Condensate to Crystalline Mineral , 2000 .

[22]  E. Gaidos.  Observational Constraints on Late Heavy Bombardment Episodes around Young Solar Analogs , 1999 .

[23]  F. Allard,et al.  The NextGen Model Atmosphere Grid for 3000 ≤ Teff ≤ 10,000 K , 1998, astro-ph/9807286.

[24]  T. Forveille,et al.  Inhibition of giant-planet formation by rapid gas depletion around young stars , 1995, Nature.

[25]  M. Hanner,et al.  The 8-13 micron spectra of comets and the composition of silicate grains , 1994 .

[26]  M. Feast,et al.  South galactic cap G and K stars with infrared excesses , 1991 .

[27]  R. Stencel,et al.  A survey for infrared excesses among high galactic latitude SAO stars , 1991 .

[28]  H. Aumann,et al.  Search for Vega-like nearby stars with 12 micron excess , 1991 .

[29]  D. Cox.  The Diffuse Interstellar Medium , 1990 .

[30]  F. Whipple,et al.  The Poynting-Robertson effect on meteor orbits , 1950 .