Lee Hartmann

Abstract: We review the general theoretical concepts and observational constraints on the distribution and evolution of water vapor and ice in protoplanetary disks, with a focus on the Solar System. Water is expected to freeze out at distances greater than 1-3 AU from solar-type central stars; more precise estimates are difficult to obtain due to uncertainties in the complex processes involved in disk evolution, including dust growth, settling, and radial drift, and the level of turbulence and viscous dissipation within disks. Interferometric observations are now providing constraints on the positions of CO snow lines, but extrapolation to the unresolved regions where water ice sublimates will require much better theoretical understanding of mass and angular momentum transport in disks as well as more refined comparison of observations with sophisticated disk models.

TL;DR: In this paper, the authors investigated the deuteration of methanol towards the high-mass star-forming region NGC 7538-IRS 1.4 mm with the IRAM-30 m antenna.

TL;DR: In this paper, the authors report the results of a sensitive K-band survey of Herbig Ae/Be disk sizes using the 85m baseline Keck Interferometer, and find a tight correlation of disk size with source luminosity R propto L^(1/2) for Ae and late Be systems.

TL;DR: In this article, the color and luminosity diagnostics based on Herschel broad-band filters were investigated to identify and discern the properties of low-mass protostars, and they found that Herschel data alone is likely a useful diagnostic of the envelope properties of young stars.