The brightest binaries:
Gespeichert in:
| Hauptverfasser: | , , |
|---|---|
| Format: | Buch |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Kluwer Academic Publ.
1998
|
| Schriftenreihe: | Astrophysics and space science library
232 |
| Schlagworte: | |
| Online-Zugang: | Inhaltsverzeichnis |
| Beschreibung: | 347 S. graph. Darst. |
| ISBN: | 079235155X |
Internformat
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| 100 | 1 | |a Vanbeveren, D. |e Verfasser |4 aut | |
| 245 | 1 | 0 | |a The brightest binaries |c by D. Vanbeveren, W. van Rensbergen and C. De Loore |
| 264 | 1 | |a Dordrecht |b Kluwer Academic Publ. |c 1998 | |
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| 490 | 1 | |a Astrophysics and space science library |v 232 | |
| 650 | 4 | |a Double stars | |
| 650 | 4 | |a Supergiant stars | |
| 700 | 1 | |a De Loore, C. |e Verfasser |4 aut | |
| 700 | 1 | |a Van Rensbergen, W. |e Verfasser |4 aut | |
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Datensatz im Suchindex
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|---|---|
| adam_text | THE BRIGHTEST BINARIES BY D. VANBEVEREN ASTROPHYSICAL INSTITUTE, VRIJE
UNIVERSITEIT BRUSSEL, BELGIUM INSTITUTE OF TECHNOLOGY LOUVAIN, LEUVEN,
BELGIUM W. VAN RENSBERGEN ASTROPHYSICAL INSTITUTE, VRIJE UNIVERSITEIT
BRUSSEL, BELGIUM AND C. DE LOORE ASTROPHYSICAL INSTITUTE, VRIJE
UNIVERSITEIT BRUSSEL, BELGIUM KLUWER ACADEMIC PUBLISHERS DORDRECHT /
BOSTON / LONDON TABLE OF CONTENTS TABLE OF CONTENTS 1 INTRODUCTION 8
LIST OF ABBREVIATIONS 10 CONSTANTS 12 CHAPTER I: MASSIVE STARS 13 1.
DEFINITION 13 2. GENERAL OBSERVATIONS 13 2.1. THE HR DIAGRAM OF MASSIVE
STARS WITH SPECTRAL TYPE O3 - M5 .... 15 2.1.1. THE EFFECTIVE
TEMPERATURE AND BOLOMETRIC CORRECTION OF MASSIVE STARS 15 2.1.2. THE
ABSOLUTE VISUAL MAGNITUDE M V OF MASSIVE STARS 18 2.1.3. THE SPECTRAL
TYPE - LUMINOSITY CLASS - MB O I - T EFF - (B-V) CALIBRATION OF MASSIVE
STARS 19 2.2. THE STELLAR WIND OF MASSIVE OB TYPE STARS 26 2.3. THE
CHEMICAL ABUNDANCES IN MASSIVE OBA TYPE STARS 31 2.4. ROTATIONAL
PROPERTIES OF OB TYPE STARS 32 2.4.1. NORMAL OB TYPE STARS 34 2.4.2.
OBE TYPE STARS 35 2.5. LBVS 36 2.6. YSGS, RSGS AND HYPERGIANTS 38 2.7.
THEWRSTARS 39 2.8. CIRCUMSTELLAR SHELLS AROUND MASSIVE STARS 42 2.9. THE
SN EXPLOSION OF A MASSIVE STAR 43 2.10. SUMMARY I , 47 CHAPTER II:
MASSIVE SINGLE STARS 49 3. THE EQUATIONS OF STELLAR STRUCTURE OF A
NON-MAGNETIC, NON-ROTATING SINGLE STAR 49 3.1. THE CONTINUITY OF MASS 50
3.2. THE PHYSICAL STATE OF THE PLASMA 50 3.2.1. HYDROSTATIC EQUILIBRIUM
50 3.2.2. NON-DEGENERACY AND DEGENERACY: DEFINITION 51 3.2.3. THE
EQUATION OF STATE OF A NON-DEGENERATE PLASMA 51 3.2.4. THE EQUATION OF
STATE OF A DEGENERATE PLASMA 52 3.2.5. THE CHANDRASEKHAR MASS LIMIT OF
DEGENERATE STARS 53 3.2.6. NEUTRON STAR MASSES 54 3.3. THE ENERGY
EQUATION 55 3.3.1. THE ENERGY GENERATION RATE BY NUCLEAR REACTIONS E 55
3.3.2. THE GRAVITATIONAL ENERGY GENERATION 59 3.4. ENERGY TRANSPORT 60
3.4.1. RADIATIVE ENERGY TRANSPORT 60 3.4.2 CONVECTIVE ENERGY TRANSPORT
AND MIXING 61 3.4.3. THE BOUNDARY BETWEEN CONVECTIVE AND RADIATIVE
LAYERS ... 63 3.5. THE TIME-VARIATION OF MASS IN EVOLUTIONARY
COMPUTATIONS 65 3.6. SUMMARY 66 3.7. SURFACE LAYERS - BOUNDARY
CONDITIONS 67 4. EVOLUTIONARY COMPUTATIONS OF NON-ROTATING MASSIVE
SINGLE STARS 70 4.1. SMALL CONVECTIVE CORE OVERSHOOTING 71 4.1.1. THE
EVOLUTION OF SINGLE STARS WITH 5 M O M 12 M O 71 4.1.2. THE
EVOLUTION OF SINGLE STARS WITH M 12 M O 76 4.2. THE EFFECT OF LARGE
CONVECTIVE CORE OVERSHOOTING 85 5. COMPARISON BETWEEN OBSERVATIONS AND
EVOLUTIONARY COMPUTATIONS OF NON-ROTATING SINGLE STARS 87 5.1.
EVOLUTIONARY COMPUTATIONS WITH SMALL CONVECTIVE CORE OVERSHOOTING 87
5.1.1. THE CORE HYDROGEN BURNING PHASE 87 5.1.2. THE POSITION OF THE
RSGS AND WR STARS IN THE HR DIAGRAM 93 5.1.3. THE PROGENITOR OF SN 1987A
94 5.1.4. THE PROGENITOR OF SN 1993J 95 5.1.5. THE OVERALL SN MORPHOLOGY
OF MASSIVE SINGLE STARS 95 5.1.6. THE BLUE HERTZSPRUNG GAP (BHG) 96
5.1.7. CHEMICAL ABUNDANCES IN EARLY B TYPE SUPERGIANTS 96 5.1.8. THE
DISTRIBUTION OF RSGS IN THE SMC 97 5.1.9. COMPARISON BETWEEN THEORETICAL
PREDICTION OF DEGENERATE STARS AND OBSERVATIONS 98 5.2. LARGE CONVECTIVE
CORE OVERSHOOTING: IS THERE A NEED? 100 6. THE EFFECT OF ROTATION ON THE
EVOLUTION OF MASSIVE SINGLE STARS 101 2 6.1. ROTATION-INDUCED MIXING IN
MASSIVE STARS 101 6.2. EVOLUTIONARY COMPUTATIONS OF ROTATING STARS 103
6.3. COMPARISON TO OBSERVATIONS 104 6.4. SUMMARY 105 CHAPTER III:
MASSIVE CLOSE BINARIES 106 7. GENERAL 106 8. THE ROCHE MODEL 106 8.1.
CIRCULARIZATION AND SYNCHRONIZATION 107 8.2 ROCHE EQUIPOTENTIALS 108
8.3. THE ROCHE LOBE OVERFLOW PROCESS 110 8.4. LIMITATIONS OF THE ROCHE
MODEL ILL 8.5. THE MASS LOSS RATE OF THE MASS LOSER DURING THE RLOF ILL
8.6. THE DIFFERENT TYPES OF UNEVOLVED MASSIVE CLOSE BINARIES 113 9. THE
MASS TRANSFER PROCESS DURING RLOF 116 9.1. DIRECT HIT VERSUS THE
FORMATION OF A KEPLERIAN DISC 116 9.2. THE SPIN-UP OF THE MASS GAINER
DUE TO MASS TRANSFER .: 117 9.3. COMPUTATION OF THE EVOLUTIONARY
BEHAVIOUR OF A MASS GAINER ... 118 9.3.1. THE STANDARD ACCRETION MODEL
120 9.3.2. THE ACCRETION INDUCED FULL MIXING MODEL 123 10. THE EVOLUTION
OF THE BINARY PERIOD IN MCBS 124 10.1. ONE OR BOTH COMPONENTS ARE LOSING
MASS BY STELLAR WIND ONLY. 124 10.2. THE VARIATION OF THE PERIOD DURING
RLOF 125 10.2.1. THE RLOF MASS LOSS DOMINATES OVER A POSSIBLE SW MASS
LOSS 126 10.2.1.1. CONSERVATIVE RLOF 126 10.2.1.2. NON-CONSERVATIVE RLOF
127 10.2.1.3. MERGERS 131 10.2.2. THE RLOF AND THE SW MASS LOSS RATES
ARE COMPARABLE .... 132 11. THE EFFECT OF THE SUPERNOVA EXPLOSION OF ONE
OF THE COMPONENTS 132 12. EVOLUTIONARY COMPUTATIONS OF MASSIVE CLOSE
BINARIES 137 12.1. THE EVOLUTION OF THE PRIMARY BEFORE AND DURING ITS
RLOF 139 12.1.1. MASSIVE PRIMARIES WITH INITIAL MASS 40-50 M O : CASE
B R WITH Q 0.2 139 12.1.2. MASSIVE PRIMARIES WITH INITIAL MASS 40-50
M O : CASE B R WITH Q 0.2, CASE B C AND CASE C 145 3 12.1.3. MASSIVE
PRIMARIES WITH INITIAL MASS 40-50 M O : CASE A.... 147 12.1.4. VERY
MASSIVE PRIMARIES 150 12.1.5. THE BINARY AFTER RLOF: A CHEB+OB BINARY OR
A MERGER? 151 12.2. THE EVOLUTION OF THE PRIMARY AFTER RLOF: CHEB+[OB OR
LOW MASS COMPANION] BINARIES 153 12.2.1. THE MASS OF THE CHEB COMPONENT
5 M O 154 12.2.2. THE MASS OF THE CHEB COMPONENT 5 M O 156 12.2.3.
THE FINAL FATE OF PRIMARIES OF MCBS 158 12.3. THE EVOLUTION OF THE
SECONDARY IN A MCB 159 12.4. THE FORMATION AND EVOLUTION OF CONTACT
BINARIES 163 12.5. THE EVOLUTION OF A MCB AFTER THE COLLAPSE OF THE CORE
OF THE PRIMARY 165 12.6. THE EFFECT OF ROTATION ON THE EVOLUTION OF A
MCB 169 12.6.1. THE PRIMARY 169 12.6.2. THE SECONDARY 170 13. MASSIVE
BINARIES: OBSERVATIONS 170 13.1. MASSIVE OBA+OBA BINARIES 171 13.1.1.
PRE-RLOF OBA+OBA MBS 171 13.1.2. MASSIVE OBA+OBA BINARIES DURING OR
AFTER RLOF 179 13.2. WR+OB BINARIES 181 13.3. X-RAY BINARIES 184 13.3.1.
HIGH MASS X-RAY BINARIES (HMXB) 184 13.3.1.1. HMXBS WITH AN OBE TYPE
OPTICAL COMPONENT 184 13.3.1.2. STANDARD HMXBS 185 13.3.1.3. HMXB
CANDIDATES WITH A WR TYPE COMPONENT 187 13.3.2. LOW MASS X-RAY BINARIES
(LMXB) WITH A MCB HISTORY 187 13.3.3. THE FORMATION OF X-RAYS WITH
ENERGIES 1 KEV 188 13.4. RADIOPULSARS 195 13.4.1. GENERAL 195 13.4.2.
BINARY RADIO PULSARS 195 13.5. MASSIVE STAR RUNAWAYS ... 198 13.5.1. OB
TYPE RUNAWAYS 198 13.5.2. RUNAWAYS OTHER THAN OB TYPE RUNAWAYS 199 14.
COMPARISON BETWEEN THE PREDICTED EVOLUTION OF MCBS AND OBSERVATIONS 200
14.1. THE BINARIES HD 163181, HD 12323, HD 14633, HD 193516, HD25638, HD
209481, PER AND V SGR 200 14.2. WR+OB BINARIES 207 14.2.1. WR+OB SYSTEMS
WHERE RLOF/MASS TRANSFER DID NOT OCCUR 209 14.2.2. WR+OB SYSTEMS WHERE
RLOF/MASS TRANSFER DID OCCUR: V 444 CYG 211 14.2.3. WR STARS WITH A LESS
LUMINOUS OB TYPE COMPANION 218 14.2.4. WR STARS WITH A NORMAL LOW MASS
COMPANION 219 14.2.5. LATE O/EARLY B TYPE STARS WITH A (TOO) FAINT WR
TYPE COMPONENT 221 14.3. THE FORMATION OF CARBON ENHANCED OB TYPE STARS
221 14.4. THE DESCENDANTS OF CHEB+OB BINARIES 222 14.4.1. HMXBS WITH AN
OB-TYPE COMPONENT: VELA X-L, WRAY 977, CYGX-1 223 14.4.2. THE OB TYPE
RUNAWAYS OPH AND PUP 230 14.4.3. CRITICAL REMARKS 235 14.5. THE
DESCENDANTS OF OB+CC BINARIES: THE CHEB (WR)+CC CANDIDATES HD 50896, HD
197406 AND CYG X-3 : 236 14.5.1. THE FORMATION OF X-RAYS IN WR+CC
BINARIES 237 14.5.2. THE X-RAY OPACITY IN THE WIND IN HMXBS 238 14.5.3.
THE EXPECTED X-RAYS IN WR+CC BINARIES 245 14.5.4. THE FORMATION OF WR
STARS WITH A CC IN THEIR CENTER 251 14.6. THE EVOLUTION OF LMXBS:
EVIDENCE FOR MCBS WITH VERY LOW MASS RATIO 251 14.7. SN-TYPE OF A MCB
COMPONENT: SN 1987A 255 14.8. SUMMARY: THE OVERALL MCB EVOLUTIONARY
MODEL 257 CHAPTER TV: MASSIVE STAR POPULATION NUMBER SYNTHESIS 262 15.
GENERAL 262 16. OBSERVATIONS USED AS INPUT IN A POPULATION MODEL 262
16.1. THE INITIAL MASS FUNCTION (IMF) 263 16.2. THE IMF OF STARBURST
REGIONS 264 16.3. THE IMF OF MASSIVE SINGLE STARS AND OF PRIMARIES OF
MCBS 265 16.4. THE OVERALL MCB FREQUENCY IN THE SOLAR NEIGHBOURHOOD 265
16.5. THE OBSERVED MASS RATIO AND PERIOD DISTRIBUTION OF PRE-RLOF MCBS
IN THE SOLAR NEIGHBOURHOOD 269 16.5.1. THE OBSERVED MASS RATIO
DISTRIBUTION 269 16.5.1.1. METHOD OF DETERMINATION 269 16.5.1.2. O-TYPE
PRIMARIES 271 16.5.1.3. B-TYPE PRIMARIES 272 16.5.2. THE OBSERVED PERIOD
DISTRIBUTION 273 16.5.3. THE IMPLICATIONS OF SELECTION EFFECTS 274 16.6.
THE RUNAWAY VELOCITIES OF SINGLE PULSARS 275 17. THE OBSERVATIONS WHICH
NEED TO BE REPRODUCED BY A MASSIVE STAR POPULATION MODEL 279 17.1. THE
B/R, WR/O AND WC/WN NUMBER RATIOS 279 17.1.1. CONTINUOUS STAR FORMATION
REGIONS 279 17.1.2. STARBURST REGIONS 280 17.2. WR+OB BINARIES 284
17.2.1. THE WR+OB FREQUENCY 284 17.2.2. THE Q AND P DISTRIBUTION OF
WR+OB 284 17.3. O-TYPE RUNAWAYS 286 17.4. THE NUMBER OF WR STARS WITH A
COMPACT COMPANION 286 17.5. THE RADIO PULSAR POPULATION 286 17.5.1.
SOLITARY RADIO PULSARS WITH A BINARY HISTORY 286 17.5.2. THE FORMATION
RATE OF DOUBLE NEUTRON STAR SYSTEMS IN THE GALAXY 287 17.6. THE SN RATE
288 18. THE POPULATION NUMBER SYNTHESIS (PNS) MODEL 289 18.1 THE OVERALL
EVOLUTIONARY MODEL OF SINGLE STARS AND MCBS 290 18.1.1. SINGLE STARS 290
18.1.2. MCBS 294 18.2. METHOD OF COMPUTATION 297 18.3. THE PARAMETERS OF
THE PNS MODEL 298 19. PNS MODEL CALCULATIONS 301 19.1. THE EXPECTED
EVOLUTION OF THE OBSERVED GALACTIC WR+OB SAMPLE 301 19.2. THE PREDICTED
DISTRIBUTION OF STARS IN REGIONS OF CONTINUOUS STAR FORMATION WITH A
REALISTIC BINARY FORMATION FREQUENCY 303 19.2.1. THE LARGE NUMBER OF
STARS OBSERVED IN THE BLUE HERTZSPRUNG GAP (BHG) 303 19.2.2. THE
DISTRIBUTION OF O-TYPE STARS PREDICTED BY THE PNS MODEL : 304 19.2.3.
THE WR POPULATION 307 19.2.4. THE EARLY B-TYPE STAR POPULATION PREDICTED
BY THE PNS MODEL 314 19.2.5. THE THEORETICALLY EXPECTED NUMBER OF BINARY
PULSARS 316 19.2.6. THE THEORETICALLY EXPECTED NUMBER OF SINGLE PULSARS
WITH A MCB HISTORY 319 19.2.7. THE RUNAWAY VELOCITY OF SINGLE PULSARS
319 19.3. THE PREDICTED DISTRIBUTION OF STARS IN STARBURST REGIONS WITH
A REALISTIC BINARY FORMATION FREQUENCY 320 19.3.1. THE POPULATION OF
B3-B0 TYPE RAPID ROTATORS IN STARBURSTS... 322 19.3.2. THE POPULATION OF
O AND WR TYPE STARS IN STARBURSTS 322 19.3.3. THE POPULATION OF RSGS AND
WR TYPE STARS IN STARBURSTS... 326 19.3.4. COOKING RECIPE 327 19.4. THE
PREDICTED SN TYPE I B C /TYPE II RATIO IN REGIONS OF CONTINUOUS STAR
FORMATION WITH A REALISTIC BINARY FORMATION FREQUENCY 328 CONCLUDING
REMARKS 330 REFERENCES 331 INDEX I 343 NIEDERS. ISTAATS-U.UNIV.-1
BIBLIC7HEK GOTTINGEN
|
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| author | Vanbeveren, D. De Loore, C. Van Rensbergen, W. |
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| dewey-full | 523.841 |
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| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.841 |
| dewey-search | 523.841 |
| dewey-sort | 3523.841 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
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| id | DE-604.BV012968331 |
| illustrated | Illustrated |
| indexdate | 2024-07-09T18:36:56Z |
| institution | BVB |
| isbn | 079235155X |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-008833784 |
| oclc_num | 39235748 |
| open_access_boolean | |
| owner | DE-19 DE-BY-UBM DE-29T |
| owner_facet | DE-19 DE-BY-UBM DE-29T |
| physical | 347 S. graph. Darst. |
| publishDate | 1998 |
| publishDateSearch | 1998 |
| publishDateSort | 1998 |
| publisher | Kluwer Academic Publ. |
| record_format | marc |
| series | Astrophysics and space science library |
| series2 | Astrophysics and space science library |
| spelling | Vanbeveren, D. Verfasser aut The brightest binaries by D. Vanbeveren, W. van Rensbergen and C. De Loore Dordrecht Kluwer Academic Publ. 1998 347 S. graph. Darst. txt rdacontent n rdamedia nc rdacarrier Astrophysics and space science library 232 Double stars Supergiant stars De Loore, C. Verfasser aut Van Rensbergen, W. Verfasser aut Astrophysics and space science library 232 (DE-604)BV000000296 232 GBV Datenaustausch application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=008833784&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis |
| spellingShingle | Vanbeveren, D. De Loore, C. Van Rensbergen, W. The brightest binaries Astrophysics and space science library Double stars Supergiant stars |
| title | The brightest binaries |
| title_auth | The brightest binaries |
| title_exact_search | The brightest binaries |
| title_full | The brightest binaries by D. Vanbeveren, W. van Rensbergen and C. De Loore |
| title_fullStr | The brightest binaries by D. Vanbeveren, W. van Rensbergen and C. De Loore |
| title_full_unstemmed | The brightest binaries by D. Vanbeveren, W. van Rensbergen and C. De Loore |
| title_short | The brightest binaries |
| title_sort | the brightest binaries |
| topic | Double stars Supergiant stars |
| topic_facet | Double stars Supergiant stars |
| url | http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=008833784&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA |
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