thesis - IRS, The Infrared Spectrograph

More documents

Recommendations

Info

124 CHAPTER 6: Physical Conditions in PDRs around Planetary NebulaeFigure 6.4–. Comparisonof the atomicfine structure linefluxes and the incidentflux densityof the oxygen- andcarbon-rich PNe withthe theoretical PDRmodels of Kaufmanet al. (1999) andW. Latter as reportedin Fong et al. (2001)respectively. <strong>The</strong>error in G 0 is approximatelyof the sizeof the plotted symbols.Note that theoxygen-rich PN Mz 3is not plotted becauseit lies outside themodel predictions forG 0. <strong>The</strong> intensitiesof the oxygen linesfor Mz 3 (the carbonline is not observed)are also higher thanthose predicted by themodels.
6.7. Physical conditions of the PDRs 125Figure 6.5–. Comparison of the O-rich model by Kaufman et al. (1999) (dashed and solid lines) withthe observational points (triangles).Figure 6.6–. Same as in Fig. 6.5 but comparing the C-rich model of W. Latter as reported in Fonget al. (2001) with the observational points (diamonds).
Page 1 and 2:
RIJKSUNIVERSITEIT GRONINGENPhysics
Page 3 and 4:
To my parents
Page 5 and 6:
Contents1 Introduction 11.1 Evoluti
Page 7 and 8:
CONTENTSvii5 Probing AGB nucleosynt
Page 9 and 10:
1IntroductionPLANETARY NEBULAE are
Page 11 and 12:
1.1. Evolution of low and intermedi
Page 13 and 14:
1.2. Planetary Nebulae 5Flash−Dri
Page 15 and 16:
1.3. Physics in PNe 7their whole li
Page 17 and 18:
1.3. Physics in PNe 95.35 eVO IIIλ
Page 19 and 20:
1.4. Studying PNe in the infrared 1
Page 21 and 22:
2The ISO-SWS Spectrum ofPlanetary N
Page 23 and 24:
2.3. Data reduction 15Table 2.1-. C
Page 25 and 26:
2.4. Line flux discussion 17Table 2
Page 27 and 28:
2.5. The visual and the ultraviolet
Page 29:
2.6. Analysis 21Table 2.5-. Electro
Page 32 and 33:
24 CHAPTER 2: The ISO-SWS Spectrum
Page 34 and 35:
Page 36 and 37:
Page 39 and 40:
3An ISO and IUE study of PlanetaryN
Page 41 and 42:
3.3. Corrections to line fluxes 33[
Page 43 and 44:
3.4. Line fluxes 35Table 3.1-. Comp
Page 45 and 46:
Table 3.3-. IUE intensities, fluxes
Page 47 and 48:
3.5. Physical parameters 393.4.3 Op
Page 49 and 50:
3.5. Physical parameters 41Table 3.
Page 51 and 52:
3.6. Chemical abundances 43Table 3.
Page 53 and 54:
3.6. Chemical abundances 45Table 3.
Page 55:
3.7. Conclusions 47Acknowledgements
Page 58 and 59:
50 CHAPTER 4: Abundances of Planeta
Page 60 and 61:
Page 62 and 63:
Page 64 and 65:
Page 66 and 67:
Page 68 and 69:
Page 70 and 71:
Page 72 and 73:
Page 74 and 75:
Page 77 and 78:
5Probing AGB nucleosynthesis viaacc
Page 79 and 80:
5.1. Introduction 71about the synth
Page 81 and 82: Table 5.2-. Radius, Zanstra tempera
Page 83 and 84: 5.3. Accurate abundances of ISO-obs
Page 85 and 86: 5.3. Accurate abundances of ISO-obs
Page 87 and 88: 5.4. Nucleosynthesis in low- and in
Page 89 and 90: 5.5. Synthetic TP-AGB calculations
Page 91 and 92: 5.6. Comparison between models and
Page 111 and 112: 5.7. Summary and conclusions 103Fig
Page 113 and 114: 5.7. Summary and conclusions 105A s
Page 115 and 116: 6Physical Conditions in PDRs around
Page 117 and 118: 6.2. Observations 109are not promin
Page 119 and 120: 6.4. General parameters of the PNe
Page 121 and 122: 6.4. General parameters of the PNe
Page 123 and 124: Table 6.3-. Radius, Zanstra tempera
Page 125 and 126: 6.6. Lines fluxes 117Figure 6.2-. S
Page 127 and 128: 6.7. Physical conditions of the PDR
Page 129 and 130: 6.7. Physical conditions of the PDR
Page 131: 6.7. Physical conditions of the PDR
Page 135 and 136: 6.8. PDRs versus Shocks 127Figure 6
Page 137 and 138: 6.10. Atomic, ionized and molecular
Page 139 and 140: 6.10. Atomic, ionized and molecular
Page 141 and 142: 6.11. General discussion 133Table 6
Page 143 and 144: 6.11. General discussion 135Figure
Page 145 and 146: 6.12. Summary and Conclusions 137su
Page 147 and 148: 7Conclusions and future workTHE res
Page 149 and 150: 141• PNe with He/H > 0.14. The st
Page 151 and 152: 143HERSCHEL The launch of this sate
Page 153 and 154: Nederlandse SamenvattingSTERREN wor
Page 155 and 156: Nederlandse Samenvatting 147Figuur
Page 157 and 158: Nederlandse Samenvatting 149PHOTOIO
Page 159 and 160: Nederlandse Samenvatting 151Figuur
Page 161 and 162: Nederlandse Samenvatting 153infraro
Page 163 and 164: English SummarySTARS are born, live
Page 165 and 166: English Summary 157Figure 2-. Two e
Page 167 and 168: English Summary 159PHOTOIONIZATIONR
Page 169 and 170: English Summary 161Figure 5-. Spect
Page 171 and 172: English Summary 163all) stages of i
Page 173 and 174: BibliographyAcker A., Marcout J., O
Page 175 and 176: BIBLIOGRAPHY 167Henry R.B.C., Kwitt
Page 177 and 178: BIBLIOGRAPHY 169Pottasch S.R., Bern
Page 179 and 180: List of PublicationsPublications in
Page 181 and 182: AcknowledgementsI could easily writ
Page 183:
Acknowledgements 175sense of humor,
show all

thesis - IRS, The Infrared Spectrograph

Create successful ePaper yourself

Delete template?

Save as template?