Extragalactic astronomy and cosmology: an introduction
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| Main Author: | |
|---|---|
| Format: | Book |
| Language: | English |
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Berlin [u.a.]
Springer
2015
|
| Edition: | 2. ed. |
| Subjects: | |
| Online Access: | Inhaltstext Inhaltsverzeichnis |
| Physical Description: | XVIII, 626 S. zahlr. Ill., graph. Darst. 235 mm x 155 mm |
| ISBN: | 9783642540820 9783642540837 9783662500606 |
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| 100 | 1 | |a Schneider, Peter |d 1958- |e Verfasser |0 (DE-588)121313336 |4 aut | |
| 245 | 1 | 0 | |a Extragalactic astronomy and cosmology |b an introduction |c Peter Schneider |
| 250 | |a 2. ed. | ||
| 264 | 1 | |a Berlin [u.a.] |b Springer |c 2015 | |
| 300 | |a XVIII, 626 S. |b zahlr. Ill., graph. Darst. |c 235 mm x 155 mm | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b n |2 rdamedia | ||
| 338 | |b nc |2 rdacarrier | ||
| 650 | 0 | 7 | |a Kosmologie |0 (DE-588)4114294-9 |2 gnd |9 rswk-swf |
| 650 | 0 | 7 | |a Astronomie |0 (DE-588)4003311-9 |2 gnd |9 rswk-swf |
| 650 | 0 | 7 | |a Galaxie |0 (DE-588)4057375-8 |2 gnd |9 rswk-swf |
| 650 | 0 | 7 | |a Extragalaktisches Objekt |0 (DE-588)4483815-3 |2 gnd |9 rswk-swf |
| 655 | 7 | |0 (DE-588)4123623-3 |a Lehrbuch |2 gnd-content | |
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| 689 | 0 | 1 | |a Extragalaktisches Objekt |0 (DE-588)4483815-3 |D s |
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| 856 | 4 | 2 | |m Digitalisierung UB Regensburg - ADAM Catalogue Enrichment |q application/pdf |u http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=027440691&sequence=000002&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA |3 Inhaltsverzeichnis |
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| _version_ | 1806328658948784128 |
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| adam_text |
Contents
Introduction
and overview
. 1
1.1
Introduction
. 1
1.2
Overview
. 5
1.2.1
Our Milky Way as a galaxy
. 5
1.2.2
The world of galaxies
. 8
1.2.3
The Hubble expansion of the Universe
. 9
1.2.4
Active galaxies and starburst galaxies
. 10
1.2.5
Voids, clusters of galaxies, and dark matter
. 11
1.2.6
World models and the thermal history of the Universe
. 15
1.2.7
Structure formation and galaxy evolution
. 17
1.2.8
Cosmology as a triumph of the human mind
. 18
1.2.9
Astrophysics
&
Physics
. 18
1.3
The tools of extragalactic astronomy
. 19
1.3.1
Radio telescopes
. 20
1.3.2
Infrared telescopes
. 24
1.3.3
Optical telescopes
. 28
1.3.4
UV telescopes
. 34
1.3.5
X-ray telescopes
. 35
1.3.6
Gamma-ray telescopes
. 37
1.4
Surveys
. 40
1.5
Problems
. 42
The Milky Way as a galaxy
. 45
2.1
Galactic coordinates
. 45
2.2
Determination of distances within our Galaxy
. 46
2.2.1
Trigonometric parallax
. 47
2.2.2
Proper motions
. 48
2.2.3
Moving cluster parallax
. 48
2.2.4
Photometric distance; extinction and reddening
. 49
2.2.5
Spectroscopie
distance
. 52
2.2.6
Distances of visual binary stars
. 53
2.2.7
Distances of pulsating stars
. 53
2.3
The structure of the Galaxy
. 54
2.3.1
The Galactic disk: Distribution of stars
. 55
2.3.2
The Galactic disk: chemical composition and age;
supernovae
. 56
2.3.3
The Galactic disk: dust and gas
. 59
2.3.4
Cosmic rays
. 61
2.3.5
The Galactic bulge
. 64
2.3.6
The stellar halo
. 66
2.3.7
The gaseous halo
. 67
2.3.8
The distance to the Galactic center
. 69
xi
Contents
2.4
Kinematics of the Galaxy
. 70
2.4.1
Determination of the velocity of the Sun
. 71
2.4.2
The rotation curve of the Galaxy
. 73
2.4.3
The gravitational potential of the Galaxy
. 77
2.5
The Galactic microlensing effect: The quest for compact dark matter
. 77
2.5.1
The gravitational lensing effect I
. 78
2.5.2
Galactic microlensing effect
. 81
2.5.3
Surveys and results
. 84
2.5.4
Variations and extensions
. 87
2.6
The Galactic center
. 89
2.6.1
Where is the Galactic center?
. 89
2.6.2
The central star cluster
. 91
2.6.3
A black hole in the center of the Milky Way
. 92
2.6.4
The proper motion of Sgr A*
. 93
2.6.5
Flares from the Galactic center
. 95
2.6.6
Hypervelocity stars in the Galaxy
. 97
2.7
Problems
. 100
3
The world of galaxies
. 101
3.1
Classification
. 102
3.1.1
Morphological classification: The Hubble sequence
. 103
3.1.2
Other types of galaxies
. 103
3.1.3
The bimodal color distribution of galaxies
. 105
3.2
Elliptical Galaxies
. 108
3.2.1
Classification
. 108
3.2.2
Brightness profile
. 108
3.2.3
Composition of elliptical galaxies
. 110
3.2.4
Dynamics of elliptical galaxies
.
Ill
3.2.5
Indicators of a complex evolution
. 114
3.3
Spiral galaxies
. 116
3.3.1
Trends in the sequence of spirals
. 116
3.3.2
Brightness profile
. 117
3.3.3
The Schmidt-Kenmcutt law of star formation
. 120
3.3.4
Rotation curves and dark matter
. 122
3.3.5
Stellar populations and gas fraction
. 124
3.3.6
Spiral structure
. 125
3.3.7
Halo gas in spirals
. 126
3.4
Scaling relations
. 127
3.4.1
The Tully-Fisher relation
. 128
3.4.2
The Faber-Jackson relation
. 130
3.4.3
The fundamental plane
. 130
3.4.4
Dn
-σ
relation
. 132
3.4.5
Summary: Properties of galaxies on the Hubble sequence
. 132
3.5
Population synthesis
. 133
3.5.1
Model assumptions
. 133
3.5.2
Evolutionary tracks in the HRD; integrated spectrum
. 134
3.5.3
Color evolution
. 135
3.5.4
Star formation history and galaxy colors
. 135
3.5.5
Metallicity, dust, and Hll regions
. 136
3.5.6
The spectra of galaxies
. 137
3.5.7
Summary
. 138
3.6
The population of luminous galaxies
. 139
Contents xiii
3
.7
Chemical evolution of galaxies
. 142
3.8
Black holes in the centers of galaxies
. 144
3.8.1
The search for supennassive black holes
. 144
3.8.2
Examples for SMBHs in galaxies
. 145
3.8.3
Correlation between SMBH mass and galaxy properties
. 146
3.9
Extragalactic distance determination
. 148
3.9.1
Distance of the LMC
. 150
3.9.2
The Cepheid distance
. 151
3.9.3
Tip of the Red Giant Branch
. 152
3.9.4 Supernovae
Type la
. 152
3.9.5
Secondary distance indicators
. 153
3.9.6
The Hubble Constant
. 154
3.10
Luminosity function of galaxies
. 155
3.10.1
The Schechter luminosity function
. 155
3.10.2
More accurate luminosity and mass functions
. 157
3.11
Galaxies as gravitational lenses
. 158
3.11.1
The gravitational lens effect—Part II
. 158
3.11.2
Simple models
. 160
3.11.3
Examplesfor gravitational lenses
. 162
3.11.4
Applications of the lens effect
. 166
3.12
Problems
. 170
4
Cosmology I: Homogeneous
isotropie
world models
. 173
4.1
Introduction and fundamental observations
. 173
4.1.1
Fundamental cosmological observations
. 174
4.1.2
Simple conclusions
. 174
4.2
An expanding universe
. 177
4.2.1
Newtonian cosmology
. 177
4.2.2
Kinematics of the Universe
. 177
4.2.3
Dynamics of the expansion
. 178
4.2.4
Modifications due to General Relativity
. 179
4.2.5
The components of matter in the Universe
. 180
4.2.6
"Derivation" of the expansion equation
. 181
4.2.7
Discussion of the expansion equations
. 182
4.3
Consequences of the
Friedmann
expansion
. 183
4.3.1
The necessity of a Big Bang
. 184
4.3.2
Redshift
. 186
4.3.3
Distances in cosmology
. 188
4.3.4
Special case: The Einstem-de Sitter model
. 190
4.3.5
Summary
. 191
4.4
Thermal history of the Universe
. 192
4.4.1
The Standard Model of particle physics
. 193
4.4.2
Expansion in the radiation-dominated phase
. 194
4.4.3
Decoupling of neutrinos
. 194
4.4.4
Pair annihilation
. 195
4.4.5
Primordial nucleosynthesis
. 196
4.4.6
WTMPs as dark matter particles
. 199
4.4.7
Recombination
. 201
4.4.8
Summary
. 204
Contents
4.5
Achievements and problems of the standard model
. 204
4.5.1
Achievements
. 204
4.5.2
Problems of the standard model
. 205
4.5.3
Extension of the standard model: inflation
. 207
4.6
Problems
. 209
5
Active galactic nuclei
. 211
5.1
Introduction
. 212
5.1.1
Brief history of AGNs
. 212
5.1.2
Fundamental properties of quasars
. 215
5.1.3
AGNs as radio sources: synchrotron radiation
. 215
5.1.4
Broad emission lines
. 218
5.1.5
Quasar demographics
. 218
5.2
AGN
zoology
. 219
5.2.1
QSOs
. 221
5.2.2
Seyfert
galanes
. 222
5.2.3
LINERs
. 222
5.2.4
Radio galaxies
. 222
5.2.5
OVVs
. 222
5.2.6
BL Lac objects
. 222
5.3
The central engine: a black hole
. 224
5.3.1
Why a black hole?
. 224
5.3.2
Accretion
. 225
5.3.3
Superluminal motion
. 227
5.3.4
Further arguments for SMBHs
. 229
5.3.5
A first mass estimate for the SMBH: the Eddmgton luminosity
. 230
5.4
Components of an
AGN
. 233
5.4.1
The
IR,
optical, and UV-continuum
. 233
5.4.2
The broad emission lines
. 238
5.4.3
Narrow emission lines
. 243
5.4.4
X-ray emission
. 244
5.4.5
The host galaxy
. 247
5.4.6
The black hole mass in AGNs
. 248
5.5
Family relations of AGNs
. 252
5.5.1
Unified models
. 252
5.5.2
Beaming
. 255
5.5.3
Beaming on large scales
. 256
5.5.4
Jets at higher frequencies
. 256
5.5.5
Unified models
—
summary
. 261
5.5.6
Tidal disruption events
. 262
5.6
Properties of the
AGN
population
. 263
5.6.1
The K-correction
. 263
5.6.2
The luminosity function of QSOs
. 264
5.7
Quasar absorption lines
. 268
5.8
Problems
. 271
6
Clusters and groups of galaxies
. 273
6.1
The Local Group
. 275
6.1.1
Phenomenology
. 275
6.1.2
Mass estimate
. 276
6.1.3
Other components of the Local Group
. 278
Contents xv
6.2
Optical cluster searches
. 279
6.2.1
The Abell catalog
. 279
6.2.2
Morphological classification of clusters
. 282
6.2.3
Galaxy groups
. 282
6.2.4
Modern optical cluster catalogs
. 283
6.3
Light distribution and cluster dynamics
. 286
6.3.1
Spatial distribution of galaxies
. 286
6.3.2
Dynamical mass of clusters
. 289
6.3.3
Additional remarks on cluster dynamics
. 290
6.3.4
Intergalactic stars in clusters of galaxies
. 291
6.4
Hot gas in galaxy clusters
. 293
6.4.1
General properties of the X-ray radiation
. 293
6.4.2
Models of the X-ray emission
. 296
6.4.3
Cooling "flows"
. 300
6.4.4
The Sunyaev-Zeldovich effect
. 306
6.4.5
X-ray and SZ catalogs of clusters
. 309
6.4.6
Radio relics
. 310
6.5
Scaling relations for clusters of galaxies
. 311
6.5.1
Mass-temperature relation
. 312
6.5.2
Mass-velocity dispersion relation
. 313
6.5.3
Mass-luminosity relation
. 313
6.5.4
The
Γ
-parameter
. 314
6.5.5
Redshift dependence of scaling relations
. 315
6.5.6
Near-infrared luminosity as mass indicator
. 316
6.6
Clusters of galaxies as gravitational lenses
. 317
6.6.1
Luminous arcs
. 317
6.6.2
The weak gravitational lens effect
. 322
6.7
The galaxy population in clusters
. 329
6.7.1
Luminosity function of cluster galaxies
. 329
6.7.2
The morphology-density relation
. 330
6.8
Evolutionary effects
. 335
6.9
Problems
. 339
7
Cosmology II: Inhomogeneities in the Universe
. 341
7.1
Introduction
. 341
7.2
Gravitational instability
. 342
7.2.1
Overview
. 342
7.2.2
Linear perturbation theory
. 343
7.2.3
Peculiar velocities
. 346
7.3
Description of density fluctuations
. 347
7.3.1
Correlation functions
. 348
7.3.2
The power spectrum
. 350
7.4
Evolution of density fluctuations
. 350
7.4.1
The initial power spectrum
. 350
7.4.2
Growth of density perturbations and the transfer function
. 351
7.4.3
The baryonic density fluctuations
. 354
7.5
Non-linear structure evolution
. 357
7.5.1
Model of spherical collapse
. 357
7.5.2
Number density of dark matter
halos
. 359
7.5.3
Numerical simulations of structure formation
. 361
xvi Contents
7.6
Properties of dark matter
halos
. 366
7.6.1
Profile of dark matter
halos
. 367
7.6.2
The shape and spin of
halos
. 372
7.6.3
The bias of dark matter
halos
. 374
7.7
Weak gravitational lensing studies of dark matter
halos
. 375
7.7.1
Massive clusters
. 376
7.7.2
Galaxy-galaxy lensing
. 376
7.7.3
Interpretation: The halo model
. 378
7.7.4
Masses of groups and clusters
. 380
7.8
The substructure of
halos
. 381
7.9
Origin of the density fluctuations
. 387
7.10
Problems
. 388
8
Cosmology III: The
cosmologica]
parameters
. 391
8.1
Redshift surveys of galaxies
. 392
8.1.1
Introduction
. 392
8.1.2
Redshift surveys
. 392
8.1.3
Determination of the power spectrum
. 394
8.1.4
Baryonic acoustic oscillations
. 397
8.1.5
Effect of peculiar velocities
. 399
8.1.6
Projected correlation function
. 401
8.1.7
Angular correlations of galaxies
. 405
8.1.8
Cosmic peculiar velocities
. 406
8.2
Cosmological parameters from clusters of galaxies
. 408
8.2.1
Cluster abundance
. 408
8.2.2
Mass-to-light ratio
. 412
8.2.3 Baryon
content
. 413
8.2.4
TheLSS of clusters of galaxies
. 413
8.3
High-redshift
supernovae
and the cosmological constant
. 414
8.3.1
Observing SNela at high redshifts
. 414
8.3.2
Results
. 415
8.3.3
Discussion
. 417
8.4
Cosmic shear
. 419
8.5
Origin of the Lyman-a forest
. 423
8.5.1
The homogeneous intergalactic medium
. 423
8.5.2
Phenomenology of the
Lya
forest
. 424
8.5.3
Models of the Lyman-a forest
. 425
8.5.4
The
Lya
forest as cosmological tool
. 427
8.6
Angular fluctuations of the CMB
. 429
8.6.1
Origin of the anisotropy
:
Overview
. 429
8.6.2
Description of the CMB anisotropy
. 431
8.6.3
The fluctuation spectrum
. 431
8.6.4
Observations of the CMB anisotropy
. 434
8.6.5
WMAP: Precision measurements of the CMB anisotropy
. 438
8.6.6
From WMAP to Planck
. 441
8.7
Cosmologica]
parameters
. 445
8.7.1
The standard cosmological model from CMB measurements
. 445
8.7.2
Consistency and discrepancies with other measurements
. 448
8.7.3
Extensions of the standard model
. 450
8.7.4
Cosmic harmony
. 453
8.8
Dark energy: Cosmological constant, or something else?
. 455
8.9
Problems
. 458
Contents
9
The Universe at high redshift
. 459
9.1
Galaxies at high redshift
. 460
9.1.1
Lyman-break galaxies (LBGs)
. 461
9.1.2
Photometric redshift
. 466
9.1.3
Other few-band selection techniques
. 468
9.2
Deep views of the Universe
. 470
9.2.1
Hubble Deep Fields
. 470
9.2.2
Deep fields in other wavebands
. 473
9.2.3
Natural telescopes
. 475
9.2.4
Towards the dark ages
. 477
9.3
New types of galaxies
. 481
9.3.1
Starburst galaxies
. 481
9.3.2
Extremely Red Objects (EROs)
. 484
9.3.3
Dusty star-forming galaxies
. 486
9.3.4
Damped Lyman-alpha systems
. 493
9.3.5
Lyman-alpha blobs
. 495
9.4
Properties of galaxies at high redshift
. 496
9.4.1
Demography of high-redshift galaxies
. 496
9.4.2
The color-magnitude distribution
. 499
9.4.3
The size and shape of high-redshift galaxies
. 499
9.4.4
The interstellar medium
. 503
9.5
Background radiation at smaller wavelengths
. 504
9.5.1
The
IR
background
. 505
9.5.2
Limits on the extragalactic background light from y-ray blazars
. . 506
9.5.3
The X-ray background
. 508
9.6
The cosmic star-formation history
. 510
9.6.1
Indicators of star formation
. 511
9.6.2
Redshift dependence of the star formation: The Madau diagram
. 512
9.6.3
Summary: High-redshift galaxies
. 515
9.7
Gamma-ray bursts
. 516
10
Galaxy evolution
. 521
10.1
Introduction and overview
. 522
10.2
Gas in dark matter
halos
. 525
10.2.1
The
infall
of gas during halo collapse
. 525
10.2.2
Cooling of gas
. 526
10.3
Reionization of the Universe
. 528
10.3.1
The first stars
. 529
10.3.2
The reionization process
. 531
10.3.3
Observational probes of reionization
. 534
10.4
The formation of disk galaxies
. 536
10.4.1
The contraction of gas in
halos
. 536
10.4.2
The formation of galactic disks
. 537
10.4.3
Dynamical effects in disks
. 538
10.4.4
Feedback processes
. 539
10.4.5
The formation and evolution of
supermassive
black holes
. 540
10.4.6
Cosmic downsizing
. 541
10.5
Formation of elliptical galaxies
. 541
10.5.1
Merging of
halos
and their galaxies
. 542
10.5.2
Black hole binaries
. 547
10.5.3
Environmental effects on galaxy properties
. 551
xviii Contents
10.6 Evolution
of the galaxy population: Numerical simulations
. 552
10.6.1
Numerical methods
. 553
10.6.2
Results
. 556
10.7
Evolution of the galaxy population: Semi-analytic models
. 562
10.7.1
Method for semi-analytic modeling
. 562
10.7.2
Results from semi-analytic models
. 566
11
Outlook
. 573
11.1
Continuous progress
. 573
11.2
New facilities
. 575
11.3
Challenges
. 579
A The electromagnetic radiation field
. 583
A.I Parameters of the radiation field
. 583
A.
2
Radiative transfer
. 583
A.3
Blackbody
radiation
. 584
A.
4
The magnitude scale
. 586
A.
4.1
Apparent magnitude
. 586
A.4.2 Filters and colors
. 586
A.
4.3
Absolute magnitude
. 587
A.4.4 Bolometric parameters
. 588
В
Properties of stars
. 589
B.I The parameters of stars
. 589
B.2 Spectral class, luminosity class, and the Hertzsprung-Russell diagram
. 589
B.3 Structure and evolution of stars
. 591
С
Units and constants
. 595
D
Recommended literature
. 597
D.I General textbooks
. 597
D.2 More specific literature
. 597
D.3 Review articles, current literature, and journals
. 598
E
Acronyms used
. 599
F
Solutions to problems
. 603
Index
. 615 |
| any_adam_object | 1 |
| author | Schneider, Peter 1958- |
| author_GND | (DE-588)121313336 |
| author_facet | Schneider, Peter 1958- |
| author_role | aut |
| author_sort | Schneider, Peter 1958- |
| author_variant | p s ps |
| building | Verbundindex |
| bvnumber | BV041998593 |
| classification_rvk | US 2000 |
| classification_tum | PHY 970f PHY 980f PHY 900f |
| ctrlnum | (OCoLC)897884093 (DE-599)DNB1045790303 |
| dewey-full | 523.1 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.1 |
| dewey-search | 523.1 |
| dewey-sort | 3523.1 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik Geographie |
| edition | 2. ed. |
| format | Book |
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| genre | (DE-588)4123623-3 Lehrbuch gnd-content |
| genre_facet | Lehrbuch |
| id | DE-604.BV041998593 |
| illustrated | Illustrated |
| indexdate | 2024-08-03T01:40:48Z |
| institution | BVB |
| isbn | 9783642540820 9783642540837 9783662500606 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027440691 |
| oclc_num | 897884093 |
| open_access_boolean | |
| owner | DE-355 DE-BY-UBR DE-20 DE-12 DE-703 DE-19 DE-BY-UBM DE-91G DE-BY-TUM DE-29T |
| owner_facet | DE-355 DE-BY-UBR DE-20 DE-12 DE-703 DE-19 DE-BY-UBM DE-91G DE-BY-TUM DE-29T |
| physical | XVIII, 626 S. zahlr. Ill., graph. Darst. 235 mm x 155 mm |
| publishDate | 2015 |
| publishDateSearch | 2015 |
| publishDateSort | 2015 |
| publisher | Springer |
| record_format | marc |
| spelling | Schneider, Peter 1958- Verfasser (DE-588)121313336 aut Extragalactic astronomy and cosmology an introduction Peter Schneider 2. ed. Berlin [u.a.] Springer 2015 XVIII, 626 S. zahlr. Ill., graph. Darst. 235 mm x 155 mm txt rdacontent n rdamedia nc rdacarrier Kosmologie (DE-588)4114294-9 gnd rswk-swf Astronomie (DE-588)4003311-9 gnd rswk-swf Galaxie (DE-588)4057375-8 gnd rswk-swf Extragalaktisches Objekt (DE-588)4483815-3 gnd rswk-swf (DE-588)4123623-3 Lehrbuch gnd-content Astronomie (DE-588)4003311-9 s Extragalaktisches Objekt (DE-588)4483815-3 s DE-604 Galaxie (DE-588)4057375-8 s Kosmologie (DE-588)4114294-9 s Erscheint auch als Online-Ausgabe 978-3-642-54083-7 X:MVB text/html http://deposit.dnb.de/cgi-bin/dokserv?id=4555717&prov=M&dok_var=1&dok_ext=htm Inhaltstext Digitalisierung UB Regensburg - ADAM Catalogue Enrichment application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=027440691&sequence=000002&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis |
| spellingShingle | Schneider, Peter 1958- Extragalactic astronomy and cosmology an introduction Kosmologie (DE-588)4114294-9 gnd Astronomie (DE-588)4003311-9 gnd Galaxie (DE-588)4057375-8 gnd Extragalaktisches Objekt (DE-588)4483815-3 gnd |
| subject_GND | (DE-588)4114294-9 (DE-588)4003311-9 (DE-588)4057375-8 (DE-588)4483815-3 (DE-588)4123623-3 |
| title | Extragalactic astronomy and cosmology an introduction |
| title_auth | Extragalactic astronomy and cosmology an introduction |
| title_exact_search | Extragalactic astronomy and cosmology an introduction |
| title_full | Extragalactic astronomy and cosmology an introduction Peter Schneider |
| title_fullStr | Extragalactic astronomy and cosmology an introduction Peter Schneider |
| title_full_unstemmed | Extragalactic astronomy and cosmology an introduction Peter Schneider |
| title_short | Extragalactic astronomy and cosmology |
| title_sort | extragalactic astronomy and cosmology an introduction |
| title_sub | an introduction |
| topic | Kosmologie (DE-588)4114294-9 gnd Astronomie (DE-588)4003311-9 gnd Galaxie (DE-588)4057375-8 gnd Extragalaktisches Objekt (DE-588)4483815-3 gnd |
| topic_facet | Kosmologie Astronomie Galaxie Extragalaktisches Objekt Lehrbuch |
| url | http://deposit.dnb.de/cgi-bin/dokserv?id=4555717&prov=M&dok_var=1&dok_ext=htm http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=027440691&sequence=000002&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA |
| work_keys_str_mv | AT schneiderpeter extragalacticastronomyandcosmologyanintroduction |