Observational Constraints on The Evolution of Dust in ...

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46 New Young Stellar Population in Serpens # ID a c2d ID α b 2µm−24µm Spectral Type A V Obs c A V Cloud d A V Final SSTc2dJ (±subtype) (mag) (mag) (mag) 141 169 18295531+0049393 -0.74 A3±3 3.5 3.02 9.0 142 172 18295592+0040150 -0.85 M4±2 3.5 5.71 3.5 145 178 18295714+0033185 -0.82 G2.5±2.5 3.5 5.19 10.0 146 182 18295772+0114057 0.44 M4±2 4.0 14.05 3.0 148 206 18300178+0032162 -1.25 K7±1 2.0 5.00 7.0 149 210 18300350+0023450 -1.22 M0±1 0.0 2.25 3.5 150 222 18300861+0058466 -0.70 K5±3 0.0 2.79 5.0 Table 2.2 – Stellar parameters for the YSO candidates in Serpens a From Harvey et al. (2007b). b Obtained from a linear fit to the logarithm of the fluxes between the 2MASS K (2µm) and the MIPS1 (24µm) bands (Harvey et al. 2007b). c Extinction found in this work. d Extinction found by “c2d” over 5 ′ region. e Post-AGB stars confirmed with Spitzer IRS spectra.
Evolution of Dust in Protoplanetary Disks 47 # T eff L∗ Age B Mass B Age S Mass S (K) (L ⊙ ) (Myr) (M ⊙ ) (Myr) (M ⊙ ) 1 4900 +510 2.01 +2.39 11.60 −10.01 +13.91 1.56 +0.63 −0.48 6.10 −4.15 +11.00 −550 −1.13 2† 3270 ±145 5.24 +6.26 −2.95 3 3850 +210 −145 0.51 −0.29 +0.61 4† 3125 +145 −135 1.30 +1.55 −0.73 5† 3415 +435 −425 14.78 −8.31 +17.64 6 4350 +380 −290 1.13 +1.35 −0.64 7 3850 +210 −145 0.23 +0.27 −0.13 14 3560 ±290 0.19 +0.22 −0.10 16 3850 +210 −145 1.20 +1.44 −0.68 18† 3125 +580 −725 25.26 −14.21 +30.15 22† 3270 +435 −390 81.97 +97.83 −46.11 23† 2795 +140 −240 1.92 +2.29 −1.08 29 3560 +500 −435 0.11 −0.06 +0.14 30 3705 ±145 0.30 +0.36 −0.17 34 † 3057 +212 −177 3.24 −1.82 +3.87 35 a,† 3125 +145 −135 306.47 −172.40 +365.79 36 4350 +730 −645 1.09 +1.30 −0.61 40 2880 +535 −730 0.23 +0.27 −0.13 41 4900 +510 −550 0.01±0.01 43 3777 +500 −435 0.33 −0.18 +0.39 44 b 2990 +715 −840 47 b 3125 +580 −725 48 3057 +430 −502 0.36 +0.42 −0.20 52 5830 +370 4.76 +5.68 −260 −2.68 53 3487 +537 −430 0.13 +0.16 −0.07 55 4900 +510 −550 2.34 +2.79 −1.31 58 4060 +290 −355 1.00 +1.19 −0.56 60 3777 ±72 0.41 +0.48 −0.23 61 3850 +210 −145 1.37 +1.63 −0.77 62 5250 +580 −1190 6.70 +7.99 −3.77 66 4350 +380 −290 1.87 +2.23 −1.05 70 8720 +800 −695 12.64 −7.11 +15.09 71 3415 ±145 0.20 +0.24 −0.11 76 3705 ±145 0.21 +0.25 −0.12 77 † 3270 ±145 2.88 +3.44 −1.62 81 † 3125 +580 −725 22.08 −12.42 +26.35 82 3850 +355 −290 0.13 −0.07 +0.15 84 † 3415 +435 −425 8.33 −4.68 +9.94 85 a,† 3415 ±145 33.83 −19.03 +40.37 86 † 3057 +212 −177 22.52 +26.89 −12.67 87 3270 +435 −390 0.23 +0.28 −0.13 88 3777 +355 −290 1.48 +1.77 −0.83 89 4350 +900 −790 0.45 +0.54 −0.25 91 4060 +530 −500 2.33 +2.79 −1.31 92 3850 +210 −145 0.28 +0.34 −0.16 93 † 3560 +500 −435 4.39 +5.24 −2.47 96 3705 ±145 0.21 +0.26 −0.12 97 3560 ±290 0.16 +0.19 −0.09 98 8720 +3180 −1140 5.44 +6.49 −3.06 5.42 +10.98 −3.67 5.98 +13.19 −4.28 16.25 −10.56 +35.98 6.87 −4.99 +14.79 1.56 +3.64 −1.36 12.51 −11.01 +62.38 6.57 −4.33 +13.95 6.34 +19.20 −5.33 7.47 +19.56 −6.17 8.70 −8.02 +15.63 7.52 −6.95 +49.36 9.45 −8.31 +12.25 3.15 +7.30 −2.20 5.73 −3.81 +11.95 1.24 +3.01 −1.12 2.08 +4.18 −2.07 4.26 +4.79 −3.72 2.86 +5.90 −1.64 9.62 +21.62 −6.22 32.64 +56.97 −22.59 1.36 +7.32 −1.36 0.74 +2.08 −0.64 21.77 −19.55 +449.61 0.82 +2.26 −0.80 10.82 −6.86 +23.60 9.46 −6.18 +21.21 8.01 −5.82 +17.71 0.92 +0.13 −0.16 2.76 +5.58 −1.98 1.38 +0.18 −0.34 3.41 +8.77 −2.10 0.81 +0.11 −0.15 8.26 −5.45 +21.22 0.52±0.25 4.37 +7.90 −2.00 1.03 +0.16 −0.17 0.52 +2.19 −4.64 0.50 +0.16 −0.35 0.71 +0.15 −0.16 1.36 +0.20 −0.51 0.80 +0.11 −0.44 2.53 +0.64 −1.16 0.44 +0.27 −0.31 1.60 +0.53 −0.45 1.18 +0.15 −0.34 0.82 +0.08 −0.09 1.05 +0.17 −0.16 2.19 +1.17 −0.56 1.44 +0.25 −0.19 0.38 +0.14 −0.11 0.68 +0.11 −0.16 0.72 +0.13 −0.22 0.28 +0.41 −0.21 0.97 +0.31 −0.14 1.00 +0.32 −0.42 1.28 +0.59 −0.24 0.85 +0.10 −0.15 0.68 +0.11 −0.16 0.51 +0.24 −0.25 7.80 −4.83 +46.64 3.41 +6.76 −1.63 3.68 +14.43 −3.46 2.86 +2.86 −2.80 3.79 +14.75 −2.02 1.57 +0.43 −0.44 0.57 +0.22 −0.11 1.13 +0.19 −0.37 0.59 +0.19 −0.12 0.37 +0.22 −0.12 0.55 +0.20 −0.09 0.36 +0.29 −0.19 0.46 +0.12 −0.09 1.13 +0.03 −0.67 0.31 +0.31 −0.30 0.52 +0.39 −0.23 2.47 +2.47 −2.40 0.35 +0.35 −0.30 12.00 +9.69 −6.27 1.50 +0.46 −0.28 5.35 −3.54 +34.68 0.33 +0.35 −0.17 4.98 +9.13 −3.47 1.66 +0.41 −0.53 2.39 +3.91 −2.33 0.76 +0.37 −0.30 2.89 +6.01 −1.71 0.52 +0.06 −0.05 2.07±0.41 0.66±0.09 3.87 +4.94 −3.63 2.09 +0.49 −1.52 2.13 +3.49 −2.13 1.12 +0.42 −0.39 8.18±2.21 2.09±0.19 2.94 +3.96 −0.93 0.31±0.06 5.40 +11.80 −2.90 0.46 +0.13 −0.09 19.65 +57.48 −13.69 0.58 +0.09 −0.22 2.57 +2.13 −2.57 0.25 +0.21 −0.08 1.76 +0.27 −0.27 0.66 +0.15 −0.15 13.98 −13.10 +35.23 1.00 +0.13 −0.61 2.53±0.20 1.13±0.37 5.82 −3.42 +14.61 0.58 +0.22 −0.12 5.23 −2.76 +11.50 4.94 +9.43 −2.37 3.79 +3.79 −3.79 0.46 +0.13 −0.09 0.37 +0.22 −0.12 2.73 +2.73 −2.73
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Observational <str
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Promotiecommissie Promotor: Co-Prom
Page 6 and 7: Cover Artwork: Roderik Overzier
Page 8 and 9: viii Chapter 3. YSOs in the Lupus M
Page 10 and 11: x Publications 217 Acknowledgments
Page 12 and 13: 2 Introduction planets may eventual
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Page 16 and 17: 6 Introduction 1.3.1.1 Disk Observa
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Page 28 and 29: 18 Introduction the potential to ch
Page 30 and 31: 20 Introduction Gorti, U., Dullemon
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Evolution of Dust in Protoplanetary
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A. Background Sources 111 Table 4.3
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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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Resumo em Português Restrições O
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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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