... The stars in the central, structureless region and the material (stars, gas, and dust) in the outer disk rotate in two different planes that are nearly perpendicular to each other. ...
... With the IR images taken at Tirgo it is possible to derive their age, age spread, dust contents, distance and the presence of proto-planetary disks. ...
... Protoplanetary disks around Pre-MS stars . Evolution of disk mass during PMS . Evolution of dust properties . ... Evolution of disk mass during PMS . Evolution of dust properties . Evolution of gas/dust ratio (followup). ...
... Ae and T Tauri disks and reveal highly pro- cessed dust (Beckwith & Sargent 1991 ... With the ducial value of the dust emissivity, we derive a disk mass of 0.01 M . ... of a circumstellar disk, is surrounding MWC 1080 A. A cooler dust compo- nent is ...
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... With the large AV implied by the molecular observa tions the K band emission may be better explained by a hot dust envelope or disk close to the stellar source rather than by intrinsic stellar emission. ...
... The object is remarkable because of its low estimated mass and age and because it is associated with a mid-infrared source, an indication of a surrounding dusty disk. Based on the comparison of our spectrum with similar spectra of field M-dwarfs...
... Similar structures were found by Hubble in Orion, and have been interpreted as gas and dust evaporation from possibly protoplanetary disks (proplyds). ...