The formation of stars and planets
... – Derived mass: 0.1...170 M: large! • Most of accelerated mass must have been swept up from the cloud core, rather than originating in mass ejected from the star ...
... – Derived mass: 0.1...170 M: large! • Most of accelerated mass must have been swept up from the cloud core, rather than originating in mass ejected from the star ...
Observations of Water and other molecules in Protoplanetary Disk
... Small scales at large distances make resolution of planet-forming regions difficult. The bulk of the disk mass is H2, which is difficult to detect. ...
... Small scales at large distances make resolution of planet-forming regions difficult. The bulk of the disk mass is H2, which is difficult to detect. ...
NASA`s X-ray Eye on the Universe
... times Sun’s mass • SMBH size ~ our solar system (15 lt mins) • SMBH grows as material falls in ...
... times Sun’s mass • SMBH size ~ our solar system (15 lt mins) • SMBH grows as material falls in ...
