Observational Constraints on The Evolution of Dust in ...

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158 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) · · · 22.0 +11.7 −8.4 9.2 +6.1 −6.1 0.0 +2.0 −0.0 10.2 +7.4 −5.8 RWAur K3 26.1 +9.0 −9.6 0.3 +1.0 −0.0 1.5 +2.1 −0.0 0.0 +0.5 −0.0 RYTau G1 6.5 +3.8 −1.8 8.4 +1.7 −2.7 1.1 +0.8 −0.6 8.0 +1.7 −1.5 SUAur G1 20.2 +5.0 −5.4 0.0 +0.6 −0.0 1.3 +1.0 −0.9 0.0 +0.6 −0.0 UYAur K7 19.9 +6.4 −6.8 0.1 +2.6 −0.0 0.0 +1.3 −0.0 0.0 +1.9 −0.0 V710Tau M1 27.7 +14.5 −19.2 0.0 +1.6 −0.0 2.8 +2.6 −1.8 0.9 +1.45 −0.6 V773Tau K3 26.2 +24.6 −5.4 3.8 +5.9 −0.0 1.3 +2.3 −0.0 0.0 +1.8 −0.0 V836Tau K7 1.2 +3.4 −0.0 0.9 +0.8 −0.6 4.5 +1.9 −0.8 0.0 +0.9 −0.0 · · · 30.7 +48.4 −8.9 0.0 +26.6 −0.0 1.7 +9.2 −0.0 10.4 +61.5 −0.0 V955Tau K5 0.0 +1.3 −0.0 0.0 +0.9 −0.0 6.3 +2.5 −1.6 10.7 +3.1 −2.8 VYTau M0 2.5 +13.5 −0.0 0.0 +12.4 −0.0 3.3 +16.1 −0.0 0.0 +8.4 −0.0 ZZTauIRS M4.5 16.0 +6.3 −3.5 0.7 +3.0 −0.0 0.7 +2.2 −0.0 0.1 +1.2 −0.0 · · · 16.1 +8.6 −6.5 0.0 +2.0 −0.2 8.1 +6.9 −5.0 6.0 +4.7 −3.3 Upper Scorpius PBB2002 J160357.9 M2 8.2 +16.3 −2.1 0.0 +1.5 −0.0 2.1 +4.6 −0.2 0.0 +1.0 −0.0 PBB2002 J160823.2 K9 2.4 +6.2 −0.0 0.0 +5.3 −0.0 3.8 +6.2 −0.0 0.0 +1.1 −0.0 PBB2002 J160900.7 K9 17.2 +6.5 −4.5 0.5 +1.4 −0.0 3.0 +2.0 −1.6 0.0 +0.3 −0.0 PBB2002 J160959.4 M4 17.7 +31.6 −11.4 0.0 +2.7 −0.0 4.8 +3.8 −2.4 0.5 +2.5 −0.0 PBB2002 J161115.3 M1 20.3 +4.2 −12.7 0.0 +2.4 −0.0 1.9 +2.5 −1.4 0.0 +0.7 −0.0 PBB2002 J161420.2 M0 6.5 +1.4 −1.4 0.0 +0.5 −0.0 1.4 +0.9 −0.9 0.0 +0.3 −0.0 PZ99 J160357.6 K5 0.0 +3.1 −0.0 0.0 +2.8 −0.0 2.8 +5.1 −0.0 0.0 +3.2 −0.0 PZ99 J161411.0 K0 0.0 +2.0 −0.0 0.0 +4.0 −0.0 1.1 +2.1 −0.0 1.4 +4.4 −0.0 ScoPMS31 M0.5 9.6 +7.5 −11.3 0.0 +2.5 −0.0 1.9 +3.3 −1.8 3.0 +4.6 −1.6 η Chamaeleontis J0843 M3.4 27.2 +16.9 −11.0 1.1 +8.3 −0.0 4.4 +3.3 −0.0 1.5 +2.8 −0.0 RECX-5 M3.8 36.1 +23.4 −19.4 0.0 +2.9 −0.0 12.3 +8.7 −0.0 0.3 +14.8 −0.0 RECX-9 M4.4 42.9 +21.6 −34.1 0.0 +6.0 −0.0 1.9 +3.9 −1.0 8.6 +8.3 −6.7 RECX-11 K6.5 36.9 +18.1 −17.2 1.4 +3.4 −0.0 3.4 +8.4 −0.0 2.6 +4.2 −0.0 Table A.1 – Small dust composition derived using the “B2C” procedure. b a Amorphous olivine and pyroxene combined. b For each object, the first line corresponds to the warm component abundances, while the second line corresponds to the cold component abundances, when available.
A. Relative Abundances of Species 159 ID Oli/Pyr a % Ens % For % Sil % Oli/Pyr a % Sil % (1.5 µm) (1.5 µm) (1.5 µm) (1.5 µm) (6.0 µm) (6.0 µm) Serpens 1 53.7 +16.5 −23.0 3.5 +3.5 −2.4 0.0 +2.9 −0.0 1.0 +2.1 −0.0 7.8 +3.8 −0.0 0.6 +1.9 −0.0 · · · 29.3 +6.2 −15.3 6.8 +4.3 −2.8 0.2 +1.1 −0.0 0.3 +1.4 −0.0 9.7 +4.7 −4.4 5.5 +1.4 −1.6 3 43.9 +19.8 −18.6 0.2 +4.1 −0.2 2.7 +3.8 −2.1 0.0 +2.9 −0.0 15.7 +3.2 −2.8 0.0 +1.0 −0.0 · · · 32.9 +34.1 −9.9 4.9 +19.2 −5.5 0.0 +13.9 −2.9 12.7 +22.5 −5.6 10.2 +7.4 −4.7 1.8 +2.2 −0.6 6 38.2 +11.6 −7.4 1.0 +1.4 −0.0 1.0 +1.4 −0.0 0.0 +1.4 −0.0 28.8 +4.5 −5.0 4.8 +3.6 −1.8 · · · 46.1 +19.8 −20.3 4.7 +6.2 −0.0 1.2 +2.3 −0.0 2.7 +4.4 −0.0 25.4 +8.6 −7.6 3.7 +2.2 −0.0 7 75.6 +26.0 −23.9 0.0 +5.6 −0.1 3.7 +4.7 −3.0 0.0 +5.1 −0.0 0.0 +9.8 −0.0 16.1 +4.4 −13.7 · · · 6.0 +7.7 −6.0 14.1 +8.8 −11.7 0.0 +3.0 −0.1 24.7 +14.3 −19.7 25.6 +14.0 −13.9 0.0 +3.5 −2.6 9 27.4 +5.7 −7.2 3.8 +2.4 −2.1 2.5 +1.5 −2.0 0.0 +1.3 −0.0 3.6 +4.1 −0.0 3.7 +1.7 −0.0 · · · 9.4 +6.7 −6.1 0.0 +3.8 −0.8 0.0 +1.5 −0.0 7.5 +5.8 −5.2 24.4 +16.2 −14.3 2.7 +7.2 −3.2 10 37.6 +17.3 −16.8 7.2 +4.2 −3.5 5.3 +6.6 −2.9 0.2 +4.0 −0.0 31.6 +18.5 −8.3 9.5 +7.6 −4.4 · · · 39.0 +23.6 −10.3 0.0 +20.1 −0.0 3.3 +9.6 −1.3 0.0 +9.3 −0.0 14.8 +35.1 −1.2 3.6 +14.1 −0.5 14 54.7 +31.3 −20.3 4.8 +20.8 −0.0 0.0 +4.9 −0.0 0.0 +8.7 −0.0 13.5 +9.3 −5.8 12.8 +10.4 −4.0 15 51.3 +9.3 −16.1 3.0 +3.4 −1.5 0.0 +1.6 −0.0 0.8 +1.8 −0.0 1.2 +2.2 −0.0 5.0 +2.0 −0.5 · · · 34.9 +9.9 −12.2 0.0 +1.0 −0.0 5.4 +2.0 −2.1 0.0 +2.1 −0.6 14.6 +4.7 −4.6 3.0 +1.4 −1.9 21 20.2 +10.1 −12.9 0.1 +4.2 −0.0 19.2 +11.1 −9.1 0.0 +4.2 −0.0 43.3 +.6.5 −21.3 12.3 +8.6 −9.1 · · · 42.5 +22.6 −24.9 2.7 +14.8 −0.0 0.5 +3.8 −0.0 0.0 +14.2 −0.0 9.6 +8.7 −3.3 8.7 +5.2 −7.5 29 71.0 +26.0 −49.2 0.0 +9.3 −0.0 4.4 +9.4 −3.1 0.0 +7.9 −0.0 13.0 +6.4 −7. 5.6 +14.7 −3.1 30 12.5 +8.5 −6.4 12.5 +8.1 −3.4 1.3 +5.9 −0.9 1.5 +5.0 −0.8 64.2 +18.1 −47.0 0.0 +21.4 −0.0 · · · 8.0 +58.7 −19.4 9.1 +14.9 −5.1 29.6 +44.9 −24.3 11.4 +37.5 −10.3 14.0 +36.3 −10.3 2.1 +9.6 −2.3 31 15.0 +2.6 −1.5 2.5 +1.2 −0.0 3.4 +1.5 −1.3 0.4 +0.4 −0.0 76.1 +7.8 −5.4 0.6 +1.0 −0.0 · · · 24.0 +4.7 −4.0 2.3 +2.0 −0.0 0.5 +1.7 −0.0 5.4 +4.4 −2.6 9.2 +4.8 −5.2 17.6 +3.3 −4.7 36 51.9 +12.1 −12.3 1.0 +2.9 −0.6 3.3 +2.8 −2.5 0.0 +1.6 −0.0 10.8 +2.8 −2.6 9.0 +2.7 −4.8 · · · 38.1 +11.0 −14.3 0.0 +2.4 −0.0 0.0 +2.9 −0.0 0.2 +8.7 −0.0 19.6 +5.9 −7.7 0.1 +0.3 −1.4 40 41.2 +17.3 −25.0 22.5 +11.0 −8.8 17.9 +11.6 −7.4 0.0 +5.5 −0.0 4.5 +9.7 −0.2 0.0 +9.8 −0.0 · · · 18.2 +9.5 −13.8 2.1 +12.8 −1.9 13.4 +7.8 −9.8 0.0 +3.0 −0.0 0.2 +9.7 −0.0 22.3 +11.2 −12.6 41 66.6 +6.8 −58.2 3.4 +16.3 −0.0 16.4 +11.3 −8.6 0.0 +6.3 −0.0 2.6 +13.8 −0.0 0.0 +14.8 −0.0 43 42.1 +19.1 −27.0 7.1 +8.9 −5.1 2.7 +7.1 −2.0 0.0 +3.5 −0.0 37.2 +15.8 −19.3 2.0 +12.7 −0.0 48 73.3 +28.2 −35.2 0.0 +9.2 −0.0 0.0 +13.8 −0.1 1.1 +9.9 −0.7 6.0 +8.4 −2.1 9.9 +4.6 −6.9 · · · 18.7 +10.0 −17.6 0.0 +7.5 −0.1 4.1 +12.0 −3.5 8.6 +5.8 −8.1 7.4 +5.6 −4.7 7.5 +4.4 −6.6 53 30.2 +18.2 −14.6 10.1 +19.9 −5.8 0.0 +11.6 −0.0 2.3 +15.6 −0.7 32.9 +27.1 −6.7 8.1 +9.4 −5.3 55 71.0 +16.2 −26.2 0.0 +3.0 −0.0 0.0 +2.7 −0.0 1.9 +3.0 −0.0 4.2 +1.5 −0.8 2.1 +0.9 −0.7 · · · 20.5 +71.1 −20.0 15.7 +72.9 −9.9 0.0 +22.3 −0.1 4.8 +65.6 −4.2 2.9 +5.8 −1.6 1.9 +6.0 −1.8 56 44.6 +16.6 −28.5 5.0 +7.9 −2.7 1.7 +7.3 −0.5 0.0 +4.6 −0.0 29.5 +11.8 −11.8 6.1 +12.2 −0.1 · · · 29.8 +11.0 −12.0 0.0 +15.8 −0.0 1.1 +7.5 −0.0 0.0 +3.2 −0.0 19.3 +24.2 −7.9 1.6 +27.0 −0.0 57 72.0 +29.0 −40.9 10.5 +13.3 −6.6 0.0 +7.1 −0.0 0.0 +7.1 −0.0 6.5 +19.1 −0.0 0.0 +9.5 −0.0 · · · 13.1 +55.6 −4.8 0.3 +27.7 −0.0 4.5 +61.3 −0.0 1.7 +25.5 −4.5 25.1 +85.7 −3.7 17.2 +81.4 −5.0 58 29.9 +4.6 −6.7 1.0 +2.2 −0.7 7.1 +3.0 −2.1 0.0 +1.8 −0.0 28.3 +6.5 −11.5 25.4 +6.4 −8.7 · · · 57.0 +24.9 −36.3 0.0 +7.5 −0.0 0.0 +8.0 −0.0 0.0 +6.2 −0.0 4.7 +2.9 −1.4 2.8 +2.5 −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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209 interagem gravitacionalmente, 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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