We review current indirect evidence that supports the hypothesis that disks of gas and dust surround young stars in their formation stages. Current theoretical models explain this evidence, in particular the observed spectral energy distributions $\lambda$F$\sb{\lambda}\propto\lambda\sp{-\eta}$ and luminosities. We argue that a consequence of these models is a flared disk structure H(r) $\propto$ r$\sp{\rm z}$ that should be observable, yielding a relation between the flaring constant z and the spectral index $\eta$ that can be used to propose an evolutionary sequence for the geometry of such disks. We performed high resolution observations in the infrared, aimed imaging scattered radiation from dust embedded in circumstellar disks in solar type pre-main sequence stars. We used an infrared array recently developed by the Kitt Peak National Observatory, in combination with the 4 meter telescope. These observations were analyzed using different super-resolution techniques such as image motion suppression, speckle shift-and-add, contrast-ratio analysis, maximum entropy restorations, and speckle interferometry. We present the results of these studies for the star SCrA, as a case study. However, we discovered that the response function of the telescope has three peaks, with typical separations of half to one arc second, and variations in intensity and position of 30% in times as short as one minute. This unstable response sets a limit of only 2 mag/$\prime\prime\sp2$ fainter than the central star for any extended structure that can be resolved, which is brighter than the 3.75 mag/$\prime\prime\sp2$ expected for a flared disk, and thus hampers the possibility of recovering disks structures. In addition, we find that the noise in long exposure images in the infrared is proportional to the signal, possibly due to the low number of speckles at these wavelengths. On the other hand, the noise in the speckles themselves appears to be of Poisson type, but the events that make those statistics are not individual photons, but bunches of many, such that the number of photons in each event is proportional to the intensity of the source.
| Identifer | oai:union.ndltd.org:UMASS/oai:scholarworks.umass.edu:dissertations-7837 |
| Date | 01 January 1990 |
| Creators | Salas-Casales, Luis |
| Publisher | ScholarWorks@UMass Amherst |
| Source Sets | University of Massachusetts, Amherst |
| Language | English |
| Detected Language | English |
| Type | text |
| Source | Doctoral Dissertations Available from Proquest |
Page generated in 0.0024 seconds