Dust distributions in debris disks: effects of gravity, radiation pressure and collisions

By A. Krivov, T. Löhne, M. Sremčević. 2006

150 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/8756cd01e12ba449bafaabe76b539db9c000ddc2

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. S. Kenyon
2. B. Bromley
3. M. C. Wyatt
4. S. Raymond
5. Philip Armitage
6. A. Mandell
7. T. Löhne
8. A. Krivov

Citations in the corpus

• Variations on Debris Disks: Icy Planet Formation at 30-150 AU for 1-3 M☉ Main-Sequence Stars (2008, background): “…are dominated by collisional processes, the maximum mass in large grains is roughly 40 times larger (e.g., Dohnanyi1969;Williams&Wetherill1994; Kenyon & Bromley 2004c; Krivov et al. 2006), Mmax; large 0:5xm M : ð38Þ In both cases, the larger collision rate in more massive disks leads to more dust.”
• Debris disks as signposts of terrestrial planet formation (2011, methodology): “…population are drawn from previous studies that fit models of the collisional evolution of planetesimal belts to the statistics for the evolution of debris disks (Dominik & Decin 2003; Krivov et al. 2005, 2006; Wyatt et al. 2007b; Löhne et al. 2008; Wyatt 2008; Krivov 2010; Kains et al. 2011).”
• Long-Term Collisional Evolution of Debris Disks (2007, methodology): “24 (for details, see Krivov et al. 2006).”
• NEW DEBRIS DISKS AROUND YOUNG, LOW-MASS STARS DISCOVERED WITH THE SPITZER SPACE TELESCOPE (2009, unknown): “These processes are discussed in more detail in Hillenbrand et al. (2008); Krivov (2007); Krivov et al. (2007, 2006); Strubbe & Chiang (2006); Minato et al. (2006); Najita & Williams (2005); Plavchan et al. (2005); Chen et al. (2005a); Wyatt (2005, 2003); Dominik & Decin (2003); Jura et al. (1995);…”
• Collisional processes and size distribution in spatially extended debris discs (2007, methodology): “For these regions outside the parent body area, preliminary analytical and numerical results seem indeed to show that a a−3.5 slope could be a typical signature of the presence of highβ grains escaping from their birth region (Strubbe & Chiang 2006; Krivov et al. 2006)6.”