Observational Constraints on The Evolution of Dust in ...

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156 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) 04370+2559 – 3.1 +7.3 −0.0 1.2 +2.3 −0.0 0.7 +1.5 −0.0 0.0 +0.4 −0.0 04385+2550 M0 16.2 +2.3 −7.9 0.8 +1.3 −0.5 1.0 +1.9 −0.0 0.0 +0.7 −0.0 · · · 13.2 +11.7 −0.0 0.0 +2.2 −0.0 1.6 +3.3 −0.0 5.7 +11.4 −0.0 AATau K7 12.5 +10.1 −0.6 0.4 +1.0 −0.0 1.4 +1.4 −0.7 0.0 +0.7 −0.0 · · · 2.6 +19.7 −0.0 19.2 +15.3 −0.0 0.0 +24.2 −0.0 18.3 +22.4 −0.0 BPTau K7 29.9 +5.4 −7.9 1.1 +0.9 −0.6 1.0 +1.3 −0.0 0.0 +0.3 −0.0 CITau K7 2.3 +5.6 −0.0 0.0 +0.3 −0.0 2.1 +1.0 −0.0 0.0 +0.9 −0.0 · · · 14.8 +12.4 −7.1 0.3 +1.5 −0.0 3.5 +10.3 −0.0 7.5 +9.9 −0.0 CWTau K3 8.2 +1.9 −2.3 1.0 +0.7 −0.0 1.0 +1.5 −0.0 0.2 +2.4 −0.0 CoKuTau3 M1 3.3 +6.8 −0.5 0.0 +1.0 −0.0 2.7 +1.6 −1.4 0.0 +0.3 −0.0 · · · 15.2 +9.6 −6.0 5.3 +10.2 −0.0 3.8 +1.9 −2.7 0.2 +4.6 −0.0 CoKuTau4 M1.5 24.5 +3.5 −17.1 0.0 +2.7 −0.0 1.0 +2.2 −0.0 0.0 +1.0 −0.0 · · · 13.4 +8.4 −5.4 0.3 +1.3 −0.6 0.0 +1.4 −0.7 13.5 +9.1 −6.3 DDTau M3 10.6 +4.7 −2.7 2.6 +3.8 −0.0 2.5 +2.6 −0.0 0.0 +1.4 −0.0 · · · 38.7 +26.0 −23.6 9.0 +8.8 −6.1 18.5 +11.9 −8.6 0.0 +5.5 −0.0 DETau M1 11.0 +6.9 −2.4 0.4 +1.7 −0.0 3.3 +2.5 −0.0 0.0 +0.6 −0.0 · · · 51.2 +22.1 −24.7 0.3 +6.2 −0.0 4.4 +6.9 −0.0 0.7 +10.2 −0.0 DFTau M0.5 0.6 +8.0 −0.0 0.2 +2.3 −0.0 1.8 +2.1 −0.0 0.3 +3.1 −0.0 DHTau M2 2.3 +2.1 −0.3 1.8 +1.8 −0.8 5.4 +2.4 −1.2 1.5 +1.6 −0.9 · · · 32.0 +16.2 −12.3 2.5 +6.0 −1.7 3.4 +8.5 −3.1 0.0 +5.6 −1.3 DKTau M0 13.0 +3.8 −3.1 0.6 +0.9 −0.0 1.9 +1.3 −1.2 3.3 +1.3 −0.9 DLTau K7 0.1 +5.6 −1.5 0.0 +1.1 −0.0 3.0 +2.3 −1.2 5.0 +3.5 −2.2 DMTau M1 4.1 +13.6 −0.0 0.0 +1.8 −0.0 4.7 +2.3 −1.0 0.0 +1.2 −0.0 · · · 42.6 +28.1 −17.1 0.7 +8.9 −0.0 1.2 +3.6 −0.0 5.3 +12.2 −4.8 DNTau M0 3.4 +5.1 −0.0 0.0 +0.6 −0.0 2.2 +1.4 −0.6 1.4 +1.1 −0.9 · · · 33.7 +39.1 −0.0 0.2 +9.1 −0.0 0.0 +18.1 −0.0 0.0 +7.6 −0.0 DOTau M0 1.2 +8.4 −0.0 0.0 +3.8 −0.0 1.6 +2.7 −0.0 0.3 +4.0 −0.0 DPTau M0.5 35.1 +13.7 −15.8 0.0 +1.5 −0.0 1.1 +1.9 −0.0 0.0 +1.6 −0.0 · · · 20.1 +8.9 −8.0 9.8 +4.6 −5.1 3.0 +3.7 −2.1 7.7 +3.8 −3.8 DQTau M0 1.8 +1.2 −1.3 5.5 +1.7 −1.4 2.0 +1.1 −0.7 0.0 +0.6 −0.0 · · · 14.4 +12.0 −5.6 0.1 +8.7 −0.0 0.0 +8.0 −0.0 0.0 +3.3 −0.0 DRTau K7 25.0 +5.8 −5.3 0.0 +0.7 −0.0 1.0 +1.5 −0.0 0.0 +0.6 −0.0 DSTau K5 35.9 +7.1 −6.3 0.8 +2.9 −0.7 2.8 +2.3 −1.7 0.2 +1.2 −0.0 · · · 22.0 +14.7 −10.3 0.2 +3.5 −1.8 2.7 +3.3 −1.8 17.2 +14.0 −9.7 F04147+2822 M4 10.2 +6.3 −0.0 0.0 +4.3 −0.0 2.9 +2.5 −0.0 0.0 +1.4 −0.0 F04192+2647 – 3.4 +12.4 −0.0 0.1 +0.8 −0.0 3.6 +1.7 −0.8 0.0 +0.7 −0.0 · · · 19.7 +16.8 −7.4 0.0 +9.0 −1.6 14.2 +15.3 −7.1 3.7 +9.4 −4.5 F04262+2654 – 0.0 +1.0 −0.0 2.1 +2.0 −0.9 0.0 +1.2 −0.0 3.9 +2.8 −2.4 F04297+2246 – 5.7 +3.7 −1.3 0.0 +1.5 −0.0 2.6 +2.0 −1.5 0.3 +1.6 −0.0 · · · 24.7 +61.7 −6.4 3.5 +15.1 −0.0 0.1 +32.3 −0.0 0.0 +17.6 −0.0 F04297+2246A – 6.0 +4.4 −1.5 3.6 +1.8 −1.8 3.1 +1.0 −0.7 0.0 +0.9 −0.0
A. Relative Abundances <strong>of</strong> Species 157 ID SpT Oli/Pyr a % Ens % For % Sil % (0.1 µm) (0.1 µm) (0.1 µm) (0.1 µm) · · · 31.3 +15.2 −10.4 1.4 +2.8 −0.0 2.1 +2.1 −0.0 0.0 +8.2 −0.0 F04570+2520 – 2.9 +11.6 −0.0 0.1 +1.7 −0.0 0.1 +3.9 −0.0 0.0 +2.9 −0.0 · · · 0.1 +4.1 −8.8 0.0 +1.8 −1.9 0.0 +9.0 −0.0 40.0 +8.3 −30.3 FMTau M0 56.0 +14.4 −10.3 0.0 +2.4 −0.0 2.1 +2.6 −1.5 0.0 +1.7 −0.0 · · · 25.0 +46.8 −0.0 2.4 +23.7 −0.0 3.5 +4.5 −0.0 1.2 +17.8 −0.0 FNTau M5 11.3 +3.5 −2.0 4.5 +2.7 −1.4 2.7 +2.0 −1.0 0.1 +2.0 −0.2 · · · 10.6 +52.1 −0.0 9.3 +29.6 −0.0 12.6 +37.1 −0.0 0.0 +22.9 −0.0 FOTau M2 12.4 +6.8 −6.2 0.0 +4.2 −0.0 2.5 +6.5 −0.0 0.2 +3.3 −0.0 FPTau M4 25.8 +9.3 −5.8 3.7 +2.6 −2.4 0.9 +1.6 −0.4 0.0 +2.4 −0.0 · · · 8.6 +8.4 −2.5 7.2 +6.1 −3.7 2.4 +2.7 −1.7 10.1 +6.6 −0.0 FQTau M2 17.9 +15.3 −11.8 1.0 +7.1 −0.3 0.4 +3.3 −0.2 5.2 +7.0 −2.7 FSTau M1 32.5 +10.9 −9.6 1.6 +3.0 −0.6 0.3 +1.4 −0.0 1.3 +1.7 −0.6 FTTau c 20.1 +5.5 −3.9 1.0 +1.4 −0.8 2.9 +1.8 −1.5 0.0 +1.0 −0.0 · · · 14.4 +17.8 −0.0 0.0 +10.9 −0.0 0.0 +4.4 −0.0 2.9 +13.7 −0.0 FVTau K5 1.4 +6.5 −0.0 0.0 +4.8 −0.0 3.9 +3.0 −0.0 0.0 +0.8 −0.0 FXTau M1 28.2 +8.6 −5.6 3.7 +5.0 −0.0 3.4 +1.8 −1.6 0.0 +0.8 −0.0 · · · 21.1 +14.8 −3.5 0.0 +8.8 −0.0 3.9 +8.7 −0.0 4.6 +16.3 −0.0 FZTau M0 24.8 +7.5 −10.9 1.3 +2.2 −0.0 1.9 +1.0 −0.9 10.7 +2.6 −2.6 GGTau M0 9.2 +3.4 −3.7 0.9 +2.0 −0.0 1.6 +1.4 −0.0 0.0 +0.9 −0.0 GHTau M2 10.6 +3.1 −3.9 1.7 +1.7 −0.9 2.1 +1.1 −1.3 0.7 +1.4 −0.7 · · · 8.7 +4.5 −4.5 2.0 +4.1 −2.4 4.9 +5.4 −4.4 2.7 +2.7 −2.3 GITau K6 35.6 +10.0 −10.5 0.4 +3.0 −0.0 1.4 +1.3 −0.9 0.0 +0.6 −0.0 · · · 16.0 +10.5 −7.3 8.4 +5.7 −3.8 11.1 +6.0 −5.2 1.9 +5.1 −1.9 GKTau K7 64.5 +7.3 −10.7 0.0 +0.9 −0.0 3.1 +1.5 −1.3 0.0 +0.7 −0.0 GMAur K3 37.3 +9.4 −11.2 0.0 +3.2 −0.0 3.1 +2.8 −0.0 0.0 +1.3 −0.0 · · · 15.7 +29.0 −0.0 0.7 +5.5 −0.0 0.4 +29.4 −0.0 17.3 +33.6 −0.0 GOTau M0 12.0 +6.5 −7.6 0.0 +4.8 −0.0 3.4 +2.8 −2.3 0.1 +2.0 −0.0 HKTau M1 1.0 +2.9 −0.3 0.4 +2.0 −0.0 1.8 +1.3 −0.0 0.1 +1.1 −0.0 · · · 19.5 +29.6 −3.4 5.3 +10.3 −0.0 1.3 +8.8 −0.0 11.1 +54.3 −2.5 HNTau K5 13.9 +6.7 −3.7 0.0 +0.4 −0.0 0.8 +0.7 −0.0 0.0 +0.4 −0.0 HOTau M0.5 10.8 +3.7 −1.6 0.7 +1.0 −0.4 2.0 +2.6 −0.6 0.0 +0.7 −0.0 · · · 38.3 +19.0 −16.0 0.0 +1.2 −0.0 1.6 +4.0 −0.0 0.0 +2.7 −0.0 HPTau K3 57.4 +10.9 −10.6 0.0 +0.8 −0.0 1.0 +1.0 −0.0 0.0 +0.9 −0.0 Haro6-37 K7 11.4 +13.5 −7.7 0.0 +1.6 −0.0 3.4 +2.2 −1.8 3.0 +2.9 −1.8 IPTau M0 28.0 +9.2 −7.4 0.8 +2.4 −0.3 2.5 +1.4 −1.7 0.0 +0.5 −0.0 · · · 17.0 +8.1 −6.0 0.2 +7.4 −0.0 1.7 +5.7 −0.1 8.2 +5.6 −2.9 IQTau M0.5 17.3 +4.1 −4.0 0.0 +1.4 −0.0 2.0 +1.7 −1.1 0.0 +0.9 −0.0 · · · 24.3 +8.9 −6.3 0.0 +1.2 −0.0 0.7 +2.7 −0.4 1.6 +3.1 −1.0 ISTau K7 0.0 +4.1 −0.0 0.0 +3.3 −0.0 6.8 +2.9 −1.8 11.6 +3.8 −3.3 · · · 3.0 +24.8 −0.0 0.0 +31.7 −0.0 10.4 +55.5 −0.0 6.8 +66.0 −0.0 LkCa15 K5 55.9 +11.0 −15.1 0.0 +2.0 −0.0 2.7 +3.8 −0.0 0.0 +0.6 −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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207 Figura 2 - O Telescópio Espaci
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209 interagem gravitacionalmente, a
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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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