Observational Constraints on The Evolution of Dust in ...

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154 From Protoplanetary Disks to Planetary Systems ID SpT Oli/Pyr a % Ens % For % Sil % (0.1 µm) (0.1 µm) (0.1 µm) (0.1 µm) 40 M7 0.0 +8.3 −0.0 0.0 +8.4 −0.0 2.9 +4.4 −0.8 10.9 +4.6 −4.1 · · · 24.2 +15.5 −18.3 16.6 +11.2 −8.4 3.1 +16.4 −0.0 0.0 +4.8 −0.0 41 K2 0.0 +18.9 −0.0 6.3 +19.1 −0.0 3.9 +16.0 −0.0 0.8 +8.6 −0.0 43 M0.5 0.0 +13.0 −0.0 0.0 +4.0 −0.0 4.2 +5.7 −0.0 4.6 +6.1 −0.0 48 M5.5 7.0 +17.5 −0.1 0.1 +8.4 −0.0 2.0 +10.2 −0.0 0.6 +3.0 −0.6 · · · 46.0 +23.9 −40.6 5.1 +10.9 −3.3 2.5 +10.5 −1.1 0.3 +21.3 −2.3 53 M2.5 0.0 +36.7 −0.0 5.0 +26.6 −0.0 5.4 +18.5 −0.0 5.9 +20.1 −0.0 55 K2 16.9 +11.3 −4.0 1.6 +2.7 −0.0 2.3 +2.5 −0.9 0.0 +1.1 −0.0 · · · 27.7 +81.3 −23.1 4.8 +36.6 −1.1 21.5 +34.7 −14.2 0.0 +22.9 −0.0 56 – 7.8 +8.3 −2.0 1.7 +1.9 −0.8 2.5 +2.4 −0.6 1.1 +3.4 −0.0 · · · 44.4 +22.2 −17.0 1.6 +5.1 −1.0 0.0 +6.4 −0.0 2.2 +21.1 −0.0 57 – 2.2 +22.8 −0.0 0.0 +9.1 −0.0 5.7 +7.2 −1.1 3.0 +3.2 −1.4 · · · 23.0 +76.9 −5.8 0.0 +79.5 −0.0 14.4 +46.6 −10.4 0.7 +131.2 −0.0 58 K7 6.6 +3.2 −0.5 0.0 +1.0 −0.0 0.6 +1.1 −0.0 1.2 +0.7 −0.0 · · · 32.2 +16.8 −16.4 3.2 +15.6 −0.0 0.0 +3.7 −0.0 0.0 +7.2 −0.0 60 M0.5 0.0 +10.1 −0.0 9.8 +23.2 −0.0 5.2 +11.8 −0.0 0.0 +3.9 −0.0 61 M0 12.2 +7.2 −0.0 0.0 +0.6 −0.0 1.8 +1.3 −0.0 0.0 +1.1 −0.0 · · · 38.2 +3.7 −7.6 0.0 +0.8 −0.0 0.1 +0.9 −0.0 0.6 +1.7 −0.0 65 – 0.0 +2.7 −0.0 0.0 +2.0 −0.0 6.0 +2.6 −2.5 0.0 +1.0 −0.0 · · · 54.9 +56.6 −19.1 0.1 +7.9 −0.0 0.0 +6.3 −0.0 8.8 +16.2 −6.6 66 K5 2.1 +8.1 −0.0 0.0 +1.6 −0.0 0.1 +1.5 −0.0 0.8 +2.4 −0.0 · · · 33.5 +10.5 −16.5 3.9 +16.1 −0.0 4.2 +14.3 −0.0 0.0 +4.9 −0.0 71 M3 6.4 +28.2 −0.0 0.0 +1.8 −0.0 2.3 +6.8 −0.0 0.8 +8.7 −0.0 74 – 0.0 +5.1 −0.0 0.0 +1.7 −0.0 6.3 +3.7 −2.8 13.4 +4.8 −6.3 · · · 50.7 +33.8 −19.5 0.1 +11.1 −0.0 0.1 +6.4 −0.0 0.0 +29.4 −0.0 75 – 0.0 +72.5 −0.0 0.0 +10.2 −0.0 4.1 +28.5 −0.0 0.1 +20.2 −0.0 76 M1 5.3 +9.6 −3.4 0.0 +2.8 −0.0 2.6 +3.3 −0.0 1.9 +3.1 −0.0 · · · 41.8 +17.5 −23.6 3.6 +4.5 −1.9 0.0 +3.3 −0.0 0.0 +2.8 −0.0 80 – 0.3 +1.2 −0.0 0.0 +0.2 −0.0 1.2 +0.5 −0.0 0.0 +0.4 −0.0 · · · 6.4 +50.4 −0.0 8.3 +29.8 −0.0 0.6 +12.4 −0.0 7.4 +34.2 −0.0 81 M5 10.7 +2.8 −0.0 0.0 +0.8 −0.0 0.0 +0.4 −0.0 4.3 +1.2 −0.0 · · · 45.4 +6.2 −5.1 0.0 +1.1 −0.0 0.0 +0.4 −0.0 0.0 +1.5 −0.0 86 M5.5 15.7 +3.1 −1.7 0.0 +0.5 −0.0 0.8 +0.7 −0.0 0.0 +0.2 −0.0 · · · 26.7 +83.1 −0.0 12.2 +28.5 −0.0 0.0 +38.4 −0.0 1.9 +14.8 −0.0 88 M0.5 0.0 +5.0 −0.0 0.0 +1.0 −0.0 8.6 +4.4 −0.0 0.0 +0.4 −0.0 · · · 6.0 +30.9 −10.0 0.7 +37.8 −9.0 33.3 +22.2 −13.7 6.0 +31.7 −9.2 89 K5 0.0 +0.7 −0.0 0.0 +0.2 −0.0 2.6 +1.6 −1.0 1.6 +0.7 −0.0 90 – 26.0 +20.9 −12.1 0.0 +4.1 −0.1 3.0 +4.4 −1.6 0.0 +2.7 −0.0 · · · 31.1 +65.4 −0.0 7.5 +13.4 −1.4 8.5 +51.3 −0.0 0.7 +21.3 −0.0 92 M0 1.1 +9.7 −0.0 0.0 +0.9 −0.0 4.8 +4.8 −0.0 2.3 +5.3 −0.1 · · · 19.6 +9.7 −7.1 0.8 +3.4 −0.0 0.2 +9.0 −0.0 3.0 +4.6 −0.0
A. Relative Abundances <strong>of</strong> Species 155 ID SpT Oli/Pyr a % Ens % For % Sil % (0.1 µm) (0.1 µm) (0.1 µm) (0.1 µm) 96 M1 18.2 +8.7 −11.8 2.6 +3.8 −2.0 2.8 +4.6 −1.6 0.0 +5.9 −0.0 100 – 0.0 +29.3 −0.0 0.0 +12.0 −0.0 2.8 +42.3 −0.0 0.5 +35.5 −0.0 101 – 24.1 +26.6 −6.9 0.0 +4.1 −0.0 2.0 +3.2 −1.4 1.0 +4.2 −0.0 · · · 48.0 +7.1 −19.8 0.0 +2.7 −0.1 0.2 +2.7 −0.0 2.5 +3.1 −1.9 103 – 0.0 +0.9 −0.0 0.0 +0.3 −0.0 2.4 +0.6 −0.0 3.2 +0.9 −0.0 · · · 11.0 +3.7 −9.1 5.8 +4.2 −2.7 0.0 +3.9 −0.0 5.8 +3.3 −1.8 104 – 1.6 +14.7 −1.1 0.9 +6.1 −0.2 3.7 +5.2 −2.3 4.3 +4.1 −1.8 106 M3 0.0 +16.0 −0.0 5.1 +23.7 −0.0 4.0 +17.1 −0.0 5.7 +34.2 −0.0 113 K7 0.0 +1.2 −0.0 0.0 +0.7 −0.0 3.3 +1.7 −0.5 4.4 +1.3 −1.9 · · · 36.9 +19.9 −14.1 2.1 +8.1 −0.0 3.6 +4.2 −1.4 0.0 +2.6 −0.0 114 F9 0.4 +5.3 −0.0 0.0 +0.5 −0.0 2.8 +1.2 −1.1 0.1 +0.8 −0.0 115 M0.5 3.5 +6.8 −2.2 0.4 +1.2 −0.2 1.5 +1.5 −0.0 0.6 +1.2 −0.0 117 K2 74.6 +32.8 −31.9 1.4 +3.6 −0.0 5.9 +2.1 −4.1 0.0 +1.6 −0.0 · · · 37.9 +14.9 −15.7 6.3 +5.5 −4.7 19.0 +9.2 −9.9 6.1 +5.3 −4.1 119 K7 0.0 +11.2 −0.0 0.7 +23.7 −0.0 1.1 +17.4 −0.0 1.9 +31.6 −0.0 122 M0 30.7 +3.5 −30.4 0.0 +7.8 −0.0 1.4 +10.5 −0.0 0.0 +7.1 −0.0 · · · 25.3 +38.5 −12.9 0.2 +7.5 −0.6 5.5 +19.7 −0.0 22.7 +36.9 −14.1 123 M0 42.0 +65.0 −19.7 0.7 +3.3 −0.0 5.4 +2.7 −3.7 0.0 +1.4 −0.0 125 M0 4.9 +13.0 −0.0 0.0 +3.3 −0.0 2.3 +2.5 −1.6 0.0 +1.9 −0.0 · · · 31.0 +10.3 −20.4 11.6 +1.5 −12.8 0.0 +0.9 −2.6 0.0 +2.5 −0.0 127 M2 1.5 +2.9 −0.0 3.4 +1.2 −2.6 0.0 +2.0 −0.0 0.9 +1.9 −0.4 129 – 0.2 +2.4 −0.0 0.0 +0.8 −0.0 0.9 +1.7 −0.0 0.0 +1.3 −0.0 137 – 40.7 +10.3 −12.0 0.8 +6.0 −0.0 0.9 +2.9 −0.0 0.0 +2.3 −0.0 142 M4 0.7 +6.3 −0.0 0.5 +2.4 −0.0 2.6 +2.3 −1.1 1.3 +2.9 −0.2 144 – 0.0 +5.3 −0.0 0.0 +2.1 −0.0 6.1 +1.6 −1.3 4.4 +2.6 −1.9 · · · 23.3 +91.2 −9.5 22.1 +33.3 −11.6 10.9 +26.9 −9.9 0.0 +41.9 −0.0 146 M4 6.8 +2.7 −1.1 0.0 +0.6 −0.0 4.4 +1.2 −1.6 2.2 +1.1 −1.1 · · · 17.2 +6.3 −2.6 0.0 +4.2 −0.0 0.0 +3.8 −0.0 0.0 +4.7 −0.0 147 – 0.0 +4.5 −0.0 0.0 +2.9 −0.0 3.3 +2.8 −1.3 1.3 +1.6 −0.9 148 K7 7.4 +15.4 −0.0 2.5 +2.7 −1.3 3.5 +3.4 −0.8 0.0 +1.0 −0.0 · · · 3.8 +36.6 −0.0 17.8 +16.9 −8.3 30.8 +24.5 −11.4 1.9 +10.7 −0.0 149 M0 37.8 +22.2 −13.3 0.7 +2.9 −0.0 1.4 +2.8 −0.9 0.0 +1.6 −0.0 · · · 41.7 +24.7 −28.1 0.0 +5.5 −0.0 4.1 +10.3 −1.5 4.4 +8.6 −3.6 Taurus 04108+2910 M0 0.1 +0.4 −0.0 0.5 +1.4 −0.0 2.9 +1.2 −1.0 0.0 +0.8 −0.0 · · · 13.2 +9.3 −5.6 0.1 +6.5 −0.0 4.0 +10.8 −0.0 0.0 +9.9 −0.0 04200+2759 – 4.7 +1.5 −2.4 0.1 +2.2 −0.0 0.4 +1.2 −0.0 0.0 +0.9 −0.0 · · · 14.3 +11.5 −7.3 1.2 +4.5 −7.9 4.2 +5.1 −3.6 3.8 +8.2 −7.2 04216+2603 M1 43.9 +15.3 −22.8 1.8 +5.4 −0.7 2.1 +3.0 −1.0 0.0 +2.2 −0.0 · · · 18.6 +27.5 −9.0 0.1 +16.8 −0.0 13.2 +31.5 −10.7 1.8 +40.3 −8.2 04303+2240 – 2.4 +9.1 −0.0 0.0 +1.7 −0.0 2.7 +3.6 −0.0 0.0 +0.7 −0.0
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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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205 Figura 1 - Ilustração do cen
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207 Figura 2 - O Telescópio Espaci
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209 interagem gravitacionalmente, a
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211 e discos são conectados, é ba
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213 uma correta separação entre a
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216 Curriculum Vitæ omy Center (ES
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218 Publications 8. c2d Spitzer-IRS
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220 Thesis Acknowledgments Liesbeth
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