High-redshift galaxies: light from the early universe
Saved in:
| Main Author: | |
|---|---|
| Format: | Book |
| Language: | English |
| Published: |
Dordrecht [u.a.]
Springer
2009
|
| Series: | Astronomy and astrophysics library
|
| Subjects: | |
| Online Access: | Inhaltsverzeichnis |
| Physical Description: | XIV, 349 S. Ill., graph. Darst. |
| ISBN: | 9783540758235 9783540758242 |
Staff View
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| adam_text | Titel: High-redshift galaxies
Autor: Appenzeller, Immo
Jahr: 2009
Contents
Part I The Context
1 Introduction................................................... 3
1.1 The Relevance of Very Distant Galaxies....................... 3
1.2 Space, Time, and Redshift.................................. 5
1.3 Historical Remarks........................................ 6
2 The Nearby Universe........................................... 11
2.1 Planets, Stars, and Black Holes.............................. 12
2.1.1 Planets........................................... 12
2.1.2 Stars............................................. 12
2.1.3 The Evolution of Low-Mass Stars.................... 21
2.1.4 The Evolution and Fate of Massive Stars............... 22
2.1.5 Exploding Stars ................................... 23
2.1.6 Stellar-Mass Black Holes ........................... 28
2.2 Galaxies................................................. 30
2.2.1 Morphology, Classification, and Dynamics............. 32
2.2.2 Size, Luminosity, and Masses........................ 38
2.2.3 Chemical Composition ............................. 41
2.2.4 The Stellar Content of Galaxies...................... 42
2.2.5 The Interstellar Medium of Galaxies.................. 47
2.2.6 Interstellar Cloud Collapse and Star Formation ......... 50
2.2.7 Galactic Nuclei.................................... 56
2.2.8 Interactions Between Galaxies....................... 61
2.3 Galaxy Clusters and Large-Scale Structure .................... 63
2.4 The Local Intergalactic Medium............................. 67
2.5 Dark Matter.............................................. 69
2.6 Dark Energy.............................................. 70
2.7 A Cosmic Inventory ....................................... 72
3 The Past and the Future ........................................ 73
3.1 The Expanding Universe.................................... 73
Contents
3.1.1 Basic Equations and Parameters...................... 73
3.1.2 Properties of the Friedmann-Lemaitre Models.......... 77
3.1.3 Some Analytic Solutions............................ 79
3.1.4 The Cosmic Expansion at Different Epochs............ 80
3.1.5 Astronomy in the Expanding Universe ................ 82
3.2 The Formation and Evolution of Structure..................... 86
3.2.1 The Origin of Structure............................. 86
3.2.2 Modeling the Evolution of Structure.................. 88
3.2.3 Observational Tests ................................ 97
3.3 The Formation of the First Stars and Galaxies..................108
3.3.1 Evolution of the Dark-Matter Halos...................108
3.3.2 Evolution of the Baryonic matter.....................Ill
3.4 The Cosmic Future ........................................116
Part II Methods and Tools
4 Basic Techniques and Their Limitations..........................121
4.1 The Information Content of Light............................122
4.2 Imaging and Photometry....................................123
4.2.1 Telescopes and Interferometers.......................123
4.2.2 Image Detectors...................................132
4.2.3 Image Reduction and Image Analysis.................135
4.2.4 Calibrations, Units, and Sensitivities..................139
4.3 Spectroscopy.............................................146
4.3.1 Spectrographs.....................................146
4.3.2 Deriving Intrinsic Luminosities and Spectra............149
4.4 Virtual Observatories and Archives...........................151
5 Finding Very Distant Galaxies...................................153
5.1 Identification Techniques for High-Redshift Objects.............153
5.1.1 Spectroscopic Methods.............................153
5.1.2 Photometric Techniques.............................154
5.1.3 Identifications Using Emission Lines..................157
5.2 Search Strategies..........................................161
5.2.1 Large-Area Surveys................................163
5.2.2 Medium Deep Surveys..............................165
5.2.3 Deep Fields.......................................166
5.2.4 Searches Using Gravitational Telescopes .............170
6 Deriving Physical Parameters ...................................175
6.1 Geometrical and Kinematical Properties.......................175
6.2 Redshifts and Distances ....................................176
6.2.1 Measuring Redshifts ...............................176
Contents
6.2.2 Distances.........................................179
6.3 Deriving Galaxy Luminosities...............................180
6.3.1 The Basic Steps ...................................180
6.3.2 Corrections for Dust Absorption......................180
6.3.3 Luminosity Functions ..............................182
6.4 Stellar Populations and Ages................................183
6.5 Mass Estimates ...........................................187
6.6 Star-Formation Rates.......................................187
6.7 Deriving the Chemical Composition..........................190
6.7.1 Abundances from H II Emission-Line Spectra..........190
6.7.2 Abundances from the Integrated Stellar Spectra.........193
6.8 Measuring Interstellar Gas and Dust Properties.................196
6.8.1 Properties and Kinematics of the Gas .................196
6.8.2 Deriving Dust Properties............................198
6.9 Probing the Distant Intergalactic Medium .....................199
6.9.1 Light Attenuation..................................200
6.9.2 Line Profile Analysis...............................202
Part III Observational Results and Their Interpretation
7 Observed Properties of High-Redshift Galaxies....................205
7.1 Starburst Galaxies.........................................205
7.1.1 Samples of Distant Starburst Galaxies.................207
7.1.2 Properties of UV-Continuum Selected Starburst Galaxies .210
7.1.3 Lya Emission Galaxies (LAEs)......................245
7.1.4 Dust-Obscured Starburst Galaxies....................256
7.2 Passively Evolving High-Redshift Galaxies....................258
7.2.1 Properties of the High-Redshift Passively Evolving
Systems ......................................... 259
7.2.2 The Space Density of Passively Evolving Galaxies......263
7.3 Quasar Host Galaxies and Radio Galaxies.....................263
7.4 The Host Galaxies of Distant Gamma-Ray Sources .............266
8 The Space Distribution of High-Redshift Galaxies .................269
8.1 The Galaxy Number Density as a Function of Distance..........269
8.2 Statistics of Galaxy Positions................................270
8.3 Progenitors of Galaxy Clusters at High Redshift................274
9 Interactions with the Intergalactic Medium.......................277
9.1 Properties of the High-Redshift IGM .........................277
9.1.1 The Intergalactic Gas After Recombination ............277
9.1.2 The Lya Forest Absorbers...........................278
9.1.3 Hot IGM Plasma at High Redshift....................281
xiv Contents
9.2 Impact of the High-Redshift Galaxies on the IGM ..............282
9.2.1 Radiative Effects...................................282
9.2.2 Galactic Winds....................................287
9.2.3 The Chemical Enrichment of the IGM.................288
9.3 Accretion of IGM Gas......................................288
9.4 Damped Lya Systems......................................290
10 Implications...................................................293
10.1 Comparison of Observations and Theoretical Predictions.........293
10.1.1 Galaxy Sizes as a Function of Redshift................294
10.1.2 The Growth of Galaxy Masses.......................295
10.1.3 The Early Chemical Evolution.......................296
10.1.4 Predicted and Observed Space Distribution.............297
10.2 Constraints on the Beginning of Star Formation ................298
10.3 Properties of the First Stars .................................299
10.4 The Passively Evolving High-Redshift Galaxies................301
10.5 Formation of the Supermassive Black Holes...................303
10.6 The Progenitors of the Present-Day Galaxies...................303
Part IV An Outlook to the Future
11 Ongoing Work.................................................311
11.1 Enlarging the Data Base....................................311
11.2 Efforts to Derive More Accurate Physical Parameters............314
11.3 Theoretical Work..........................................316
11.3.1 Improving the Spectral Synthesis Models..............316
11.3.2 Physical Processes at the End of the Dark Age..........317
12 Future Facilities and Their Opportunities.........................319
12.1 New Instrumentation.......................................319
12.1.1 New Ground-Based Telescopes ......................319
12.1.2 New Space Instrumentation..........................324
12.2 New Observational Possibilities and Their Expected Yield .......328
12.2.1 Sensitivity Gains...................................328
12.2.2 Extending the Redshift Range........................329
12.2.3 Gains from the Improved Angular Resolution ..........329
12.3 The Long-Term Future.....................................330
12.3.1 Medium and Long-Term Projects in Space.............330
12.3.2 Advances in the Detector Technologies................331
References.........................................................333
Index.............................................................345
|
| adam_txt |
Titel: High-redshift galaxies
Autor: Appenzeller, Immo
Jahr: 2009
Contents
Part I The Context
1 Introduction. 3
1.1 The Relevance of Very Distant Galaxies. 3
1.2 Space, Time, and Redshift. 5
1.3 Historical Remarks. 6
2 The Nearby Universe. 11
2.1 Planets, Stars, and Black Holes. 12
2.1.1 Planets. 12
2.1.2 Stars. 12
2.1.3 The Evolution of Low-Mass Stars. 21
2.1.4 The Evolution and Fate of Massive Stars. 22
2.1.5 Exploding Stars . 23
2.1.6 Stellar-Mass Black Holes . 28
2.2 Galaxies. 30
2.2.1 Morphology, Classification, and Dynamics. 32
2.2.2 Size, Luminosity, and Masses. 38
2.2.3 Chemical Composition . 41
2.2.4 The Stellar Content of Galaxies. 42
2.2.5 The Interstellar Medium of Galaxies. 47
2.2.6 Interstellar Cloud Collapse and Star Formation . 50
2.2.7 Galactic Nuclei. 56
2.2.8 Interactions Between Galaxies. 61
2.3 Galaxy Clusters and Large-Scale Structure . 63
2.4 The Local Intergalactic Medium. 67
2.5 Dark Matter. 69
2.6 Dark Energy. 70
2.7 A Cosmic Inventory . 72
3 The Past and the Future . 73
3.1 The Expanding Universe. 73
Contents
3.1.1 Basic Equations and Parameters. 73
3.1.2 Properties of the Friedmann-Lemaitre Models. 77
3.1.3 Some Analytic Solutions. 79
3.1.4 The Cosmic Expansion at Different Epochs. 80
3.1.5 Astronomy in the Expanding Universe . 82
3.2 The Formation and Evolution of Structure. 86
3.2.1 The Origin of Structure. 86
3.2.2 Modeling the Evolution of Structure. 88
3.2.3 Observational Tests . 97
3.3 The Formation of the First Stars and Galaxies.108
3.3.1 Evolution of the Dark-Matter Halos.108
3.3.2 Evolution of the Baryonic matter.Ill
3.4 The Cosmic Future .116
Part II Methods and Tools
4 Basic Techniques and Their Limitations.121
4.1 The Information Content of Light.122
4.2 Imaging and Photometry.123
4.2.1 Telescopes and Interferometers.123
4.2.2 Image Detectors.132
4.2.3 Image Reduction and Image Analysis.135
4.2.4 Calibrations, Units, and Sensitivities.139
4.3 Spectroscopy.146
4.3.1 Spectrographs.146
4.3.2 Deriving Intrinsic Luminosities and Spectra.149
4.4 Virtual Observatories and Archives.151
5 Finding Very Distant Galaxies.153
5.1 Identification Techniques for High-Redshift Objects.153
5.1.1 Spectroscopic Methods.153
5.1.2 Photometric Techniques.154
5.1.3 Identifications Using Emission Lines.157
5.2 Search Strategies.161
5.2.1 Large-Area Surveys.163
5.2.2 Medium Deep Surveys.165
5.2.3 Deep Fields.166
5.2.4 Searches Using "Gravitational Telescopes".170
6 Deriving Physical Parameters .175
6.1 Geometrical and Kinematical Properties.175
6.2 Redshifts and Distances .176
6.2.1 Measuring Redshifts .176
Contents
6.2.2 Distances.179
6.3 Deriving Galaxy Luminosities.180
6.3.1 The Basic Steps .180
6.3.2 Corrections for Dust Absorption.180
6.3.3 Luminosity Functions .182
6.4 Stellar Populations and Ages.183
6.5 Mass Estimates .187
6.6 Star-Formation Rates.187
6.7 Deriving the Chemical Composition.190
6.7.1 Abundances from H II Emission-Line Spectra.190
6.7.2 Abundances from the Integrated Stellar Spectra.193
6.8 Measuring Interstellar Gas and Dust Properties.196
6.8.1 Properties and Kinematics of the Gas .196
6.8.2 Deriving Dust Properties.198
6.9 Probing the Distant Intergalactic Medium .199
6.9.1 Light Attenuation.200
6.9.2 Line Profile Analysis.202
Part III Observational Results and Their Interpretation
7 Observed Properties of High-Redshift Galaxies.205
7.1 Starburst Galaxies.205
7.1.1 Samples of Distant Starburst Galaxies.207
7.1.2 Properties of UV-Continuum Selected Starburst Galaxies .210
7.1.3 Lya Emission Galaxies (LAEs).245
7.1.4 Dust-Obscured Starburst Galaxies.256
7.2 Passively Evolving High-Redshift Galaxies.258
7.2.1 Properties of the High-Redshift Passively Evolving
Systems . 259
7.2.2 The Space Density of Passively Evolving Galaxies.263
7.3 Quasar Host Galaxies and Radio Galaxies.263
7.4 The Host Galaxies of Distant Gamma-Ray Sources .266
8 The Space Distribution of High-Redshift Galaxies .269
8.1 The Galaxy Number Density as a Function of Distance.269
8.2 Statistics of Galaxy Positions.270
8.3 Progenitors of Galaxy Clusters at High Redshift.274
9 Interactions with the Intergalactic Medium.277
9.1 Properties of the High-Redshift IGM .277
9.1.1 The Intergalactic Gas After Recombination .277
9.1.2 The Lya Forest Absorbers.278
9.1.3 Hot IGM Plasma at High Redshift.281
xiv Contents
9.2 Impact of the High-Redshift Galaxies on the IGM .282
9.2.1 Radiative Effects.282
9.2.2 Galactic Winds.287
9.2.3 The Chemical Enrichment of the IGM.288
9.3 Accretion of IGM Gas.288
9.4 Damped Lya Systems.290
10 Implications.293
10.1 Comparison of Observations and Theoretical Predictions.293
10.1.1 Galaxy Sizes as a Function of Redshift.294
10.1.2 The Growth of Galaxy Masses.295
10.1.3 The Early Chemical Evolution.296
10.1.4 Predicted and Observed Space Distribution.297
10.2 Constraints on the Beginning of Star Formation .298
10.3 Properties of the First Stars .299
10.4 The Passively Evolving High-Redshift Galaxies.301
10.5 Formation of the Supermassive Black Holes.303
10.6 The Progenitors of the Present-Day Galaxies.303
Part IV An Outlook to the Future
11 Ongoing Work.311
11.1 Enlarging the Data Base.311
11.2 Efforts to Derive More Accurate Physical Parameters.314
11.3 Theoretical Work.316
11.3.1 Improving the Spectral Synthesis Models.316
11.3.2 Physical Processes at the End of the Dark Age.317
12 Future Facilities and Their Opportunities.319
12.1 New Instrumentation.319
12.1.1 New Ground-Based Telescopes .319
12.1.2 New Space Instrumentation.324
12.2 New Observational Possibilities and Their Expected Yield .328
12.2.1 Sensitivity Gains.328
12.2.2 Extending the Redshift Range.329
12.2.3 Gains from the Improved Angular Resolution .329
12.3 The Long-Term Future.330
12.3.1 Medium and Long-Term Projects in Space.330
12.3.2 Advances in the Detector Technologies.331
References.333
Index.345 |
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| record_format | marc |
| series2 | Astronomy and astrophysics library |
| spelling | Appenzeller, Immo 1940- Verfasser (DE-588)131650092 aut High-redshift galaxies light from the early universe Immo Appenzeller Dordrecht [u.a.] Springer 2009 XIV, 349 S. Ill., graph. Darst. txt rdacontent n rdamedia nc rdacarrier Astronomy and astrophysics library Galaxies / Observations Red shift / Observations Galaxies Observations Galaxies Evolution Red shift Observations Galaxie (DE-588)4057375-8 gnd rswk-swf Rotverschiebung (DE-588)4178556-3 gnd rswk-swf Kosmologie (DE-588)4114294-9 gnd rswk-swf Galaxie (DE-588)4057375-8 s Rotverschiebung (DE-588)4178556-3 s Kosmologie (DE-588)4114294-9 s DE-604 HBZ Datenaustausch application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=016583561&sequence=000002&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis |
| spellingShingle | Appenzeller, Immo 1940- High-redshift galaxies light from the early universe Galaxies / Observations Red shift / Observations Galaxies Observations Galaxies Evolution Red shift Observations Galaxie (DE-588)4057375-8 gnd Rotverschiebung (DE-588)4178556-3 gnd Kosmologie (DE-588)4114294-9 gnd |
| subject_GND | (DE-588)4057375-8 (DE-588)4178556-3 (DE-588)4114294-9 |
| title | High-redshift galaxies light from the early universe |
| title_auth | High-redshift galaxies light from the early universe |
| title_exact_search | High-redshift galaxies light from the early universe |
| title_exact_search_txtP | High-redshift galaxies light from the early universe |
| title_full | High-redshift galaxies light from the early universe Immo Appenzeller |
| title_fullStr | High-redshift galaxies light from the early universe Immo Appenzeller |
| title_full_unstemmed | High-redshift galaxies light from the early universe Immo Appenzeller |
| title_short | High-redshift galaxies |
| title_sort | high redshift galaxies light from the early universe |
| title_sub | light from the early universe |
| topic | Galaxies / Observations Red shift / Observations Galaxies Observations Galaxies Evolution Red shift Observations Galaxie (DE-588)4057375-8 gnd Rotverschiebung (DE-588)4178556-3 gnd Kosmologie (DE-588)4114294-9 gnd |
| topic_facet | Galaxies / Observations Red shift / Observations Galaxies Observations Galaxies Evolution Red shift Observations Galaxie Rotverschiebung Kosmologie |
| url | http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=016583561&sequence=000002&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA |
| work_keys_str_mv | AT appenzellerimmo highredshiftgalaxieslightfromtheearlyuniverse |