Computer Science
Scientific paper
Dec 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999sf99.proc..235s&link_type=abstract
Star Formation 1999, Proceedings of Star Formation 1999, held in Nagoya, Japan, June 21 - 25, 1999, Editor: T. Nakamoto, Nobeyam
Computer Science
1
Scientific paper
Recent mm/sub-mm and IR observations indicate the evidence of disk formation around not only isolated young stars but also many young stars in binary or multiple systems. We calculate spectral energy distributions (SEDs) of such young stars with disks using our passive disk model and compare the results with observational data in order to study the internal structure of disks in binaries and possible formation of planetary systems. In the calculation we consider the effects of growth and settling of dust particles in protoplanetary disks. From the results it is found that in close binary systems the disk masses are relatively low and settling of dust particles is hard to occur as compared with disks in wide binaries or around isolated stars. This is attributable to gravitational perturbation from the companion star, which disturbs formation of planetary systems in disks in close binary systems.
Nakagawa Yasuhiro
Sato Yuzuru
No associations
LandOfFree
Spectral Energy Distributions of Protoplanetary Disks: Effects of Growth and Settling of Dust Particles does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Spectral Energy Distributions of Protoplanetary Disks: Effects of Growth and Settling of Dust Particles, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral Energy Distributions of Protoplanetary Disks: Effects of Growth and Settling of Dust Particles will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1061435