A STEEPER THAN LINEAR DISK MASS–STELLAR MASS SCALING RELATION

A STEEPER THAN LINEAR DISK MASS–STELLAR MASS SCALING RELATION

The disk mass is among the most important input parameter for every planet formation model to determine the number and masses of the planets that can form. We present an ALMA 887 mu m survey of the disk population around objects from similar to 2 to 0.03 M-circle dot in the nearby similar to 2 Myr o...

Full description

Bibliographic Details
Main Authors: Pascucci, I., Testi, L., Herczeg, G. J., Long, F., Manara, C. F., Hendler, N., Mulders, G. D., Krijt, S., Ciesla, F., Henning, Th., Mohanty, S., Drabek-Maunder, E., Apai, D., Szűcs, L., Sacco, G., Olofsson, J.
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2016
Subjects:
brown dwarfs
protoplanetary disks
stars: pre-main sequence
submillimeter: planetary systems
Online Access:http://hdl.handle.net/10150/622163
http://arizona.openrepository.com/arizona/handle/10150/622163

Internet

http://hdl.handle.net/10150/622163
http://arizona.openrepository.com/arizona/handle/10150/622163

Similar Items