Observational Constraints on The Evolution of Dust in ...

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184 Spectral Energy Distributions of the Young Stars with Disks in Serpens A. The Remaining SEDs Figure A.1 – SEDs of the young stellar population with disks of Serpens. Each SED has the corresponding object ID (as in Oliveira et al. 2010) on the top left. The solid black line indicates the NextGen stellar photosphere model for the spectral type indicated on the top of each plot. Open squares are the observed photometry while the solid circles are the dereddened photometry. The visual extinction of each object can be seen on the top right. The solid gray line is the object’s IRS spectrum.
A. The Remaining SEDs 185 Figure A.2 – SEDs, continued.
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Observational <str
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Promotiecommissie Promotor: Co-Prom
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Cover Artwork: Roderik Overzier
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viii Chapter 3. YSOs in the Lupus M
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x Publications 217 Acknowledgments
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2 Introduction planets may eventual
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4 Introduction Figure 1.1 - Illustr
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6 Introduction 1.3.1.1 Disk Observa
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8 Introduction 1.3.1.3 Processes Af
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10 Introduction of them (e.g., β P
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12 Introduction responsible for dis
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14 Introduction Figure 1.4 - Eviden
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16 Introduction stars (due to spect
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18 Introduction the potential to ch
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20 Introduction Gorti, U., Dullemon
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2 Optical Characterization of a New
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Evolution of Dust in Protoplanetary
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52 YSOs in the Lupus Molecular Clou
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4 A Spitzer Survey of Protoplanetar
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A. Background Sources 111 Table 4.3
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A. Background Sources 113 Figure A.
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A. Background Sources 115 Figure A.
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118 Discovery of a Dusty Planetary
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128 From Protoplanetary Disks to Pl
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Page 226 and 227: 216 Curriculum Vitæ omy Center (ES
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Page 230 and 231: 220 Thesis Acknowledgments Liesbeth
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