'Protostars and Planets V' builds on the latest results from recent advances in ground and space-based astronomy and in numerical computing techniques to offer the most detailed and up-to-date picture of star and planet formation - including the formation and early evolution of our own solar system.For a thin disk and a high stellar UV flux, Kamp and Dullemond (2004) obtain temperatures that asymptote to several 1000 K inside 50 AU. ... et al., 2000; Johns-Krull et al, 2000) and FUSE (e.g., Wilkinson et al, 2002; Bergin et al, 2003) indicate that it decreases into the FUV domain with ... Igea and Glassgold (1999) supported this conclusion with a Monte Carlo calculation of X-ray transport through disks, anbsp;...
|Title||:||Protostars and Planets V|
|Author||:||Bo Reipurth, David Jewitt, Klaus Keil|
|Publisher||:||University of Arizona Press - 2007|