From luminous hot stars to starburst galaxies
Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their lives of a few million years with prodigious outputs of radiation and stellar winds, dramatically affecting both their evolution and environments. A detailed intro...
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| Format: | Elektronisch E-Book |
| Sprache: | English |
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Cambridge
Cambridge University Press
2008
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| Schriftenreihe: | Cambridge astrophysics
45 |
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| 024 | 7 | |a 10.1017/CBO9780511536199 |2 doi | |
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| 100 | 1 | |a Conti, P. S. |e Verfasser |4 aut | |
| 245 | 1 | 0 | |a From luminous hot stars to starburst galaxies |c Peter S. Conti, Paul A. Crowther, Claus Leitherer |
| 264 | 1 | |a Cambridge |b Cambridge University Press |c 2008 | |
| 300 | |a 1 online resource (xiii, 315 pages) | ||
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| 490 | 0 | |a Cambridge astrophysics |v 45 | |
| 500 | |a Title from publisher's bibliographic system (viewed on 05 Oct 2015) | ||
| 505 | 8 | 0 | |g 1.1 |g 1 |t Motivation |g 1.2 |g 1 |t Observed properties |g 1.3 |g 5 |t Stellar atmospheres |g 1.4 |g 5 |t Stellar winds |g 1.5 |g 7 |t Evolution of single stars |g 1.6 |g 9 |t Binaries |g 1.7 |g 10 |t Birth of massive stars and star clusters |g 1.8 |g 11 |t The interstellar environment |g 1.9 |g 12 |t From GHII regions to starburst galaxies |g 1.10 |g 14 |t Starburst phenomena |g 1.11 |g 15 |t Cosmological implications |g 2 |g 17 |t Observed properties |g 2.1 |g 17 |t Apparent and absolute magnitudes |g 2.2 |g 19 |t Distances |g 2.3 |g 21 |t Massive stars in Local Group galaxies |g 2.4 |g 35 |t Spectral classification |g 2.5 |g 45 |t Observations of rotation and magnetic fields |g 3 |g 49 |t Stellar atmospheres |g 3.1 |g 49 |t LTE atmospheres |g 3.2 |g 50 |t Non-LTE atmospheres |g 3.3 |g 61 |t Surface gravities and masses |g 3.4 |g 62 |t Surface composition |g 4 |g 67 |t Stellar winds |g 4.1 |g 67 |t Radiation pressure |g 4.2 |g 74 |t Wind velocities |g 4.3 |t Mass-loss rates |t Structure and clumping |t Influence of stellar rotation |t Evolution of single stars |t Nucleosynthesis |t Evolution to a red supergiant |t Evolution to the Wolf-Rayet stage |t Rotation and mass-loss |t Magnetic massive stars |t Core-collapse supernovae |t Binaries |t Massive binary frequency |t Binary masses |t Close binary evolution |t Interacting stellar winds |t Dust formation in WC stars |t Birth of massive stars and star clusters |t Natal precursors of OB stars |t The initial mass function |t Formation of high-mass stars |t Massive stellar clusters |t The interstellar environment |t Interstellar dust |t Ionized hydrogen regions |t Wind blown bubbles |9 |g 79 -- |g 4.4 |g 90 -- |g 4.5 |g 95 -- |g 5 |g 99 -- |g 5.1 |g 99 -- |g 5.2 |g 102 -- |g 5.3 |g 107 -- |g 5.4 |g 111 -- |g 5.5 |g 115 -- |g 5.6 |g 116 -- |g 6 |g 129 -- |g 6.1 |g 129 -- |g 6.2 |g 130 -- |g 6.3 |g 133 -- |g 6.4 |g 146 -- |g 6.5 |g 149 -- |g 7 |g 154 -- |g 7.1 |g 155 -- |g 7.2 |g 163 -- |g 7.3 |g 167 -- |g 7.4 |g 170 -- |g 8 |g 180 -- |g 8.1 |g 180 -- |g 8.2 |g 184 -- |g 8.3 |g 187 -- |
| 505 | 8 | 0 | |t Ejecta nebulae around LBVs and W-R stars |t From giant HII regions to HII galaxies |t Giant HII regions: definition and structural parameters |t 30 Doradus -- the Rosetta Stone |t Stellar population diagnostics |t HII galaxies: stellar content and relation to starbursts |t Starburst phenomena |t Definition of a starburst |t The starburst IMF |t The evolution of starbursts |t Starburst-driven superwinds |t The starburst-AGN connection |t Cosmological implications |t Population III stars |t Lyman-break galaxies |t Massive stars and cosmic abundances |t Gamma ray bursts |9 |g 8.4 |g 192 -- |g 9 |g 197 -- |g 9.1 |g 197 -- |g 9.2 |g 200 -- |g 9.3 |g 208 -- |g 9.4 |g 219 -- |g 10 |g 229 -- |g 10.1 |g 229 -- |g 10.2 |g 231 -- |g 10.3 |g 241 -- |g 10.4 |g 250 -- |g 10.5 |g 255 -- |g 11 |g 266 -- |g 11.1 |g 266 -- |g 11.2 |g 272 -- |g 11.3 |g 280 -- |g 11.4 |g 287 |
| 520 | |a Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their lives of a few million years with prodigious outputs of radiation and stellar winds, dramatically affecting both their evolution and environments. A detailed introduction to the topic, this book connects the astrophysics of massive stars with the extremes of galaxy evolution represented by starburst phenomena. A thorough discussion of the physical and wind parameters of massive stars is presented. HII galaxies, their connection to starburst galaxies, and the contribution of starburst phenomena to galaxy evolution through superwinds, are explored. The book concludes with the wider cosmological implications, including Population III stars, Lyman break galaxies and gamma-ray bursts, for each of which massive stars are believed to play a crucial role. This book is ideal for graduate students and researchers in astrophysics interested in luminous hot stars and galaxy evolution | ||
| 650 | 4 | |a Starbursts | |
| 650 | 4 | |a Gamma ray bursts | |
| 650 | 4 | |a Stars / Evolution | |
| 650 | 4 | |a Stellar winds | |
| 650 | 0 | 7 | |a Sternwind |0 (DE-588)4244849-9 |2 gnd |9 rswk-swf |
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| 700 | 1 | |a Crowther, Paul A. |e Sonstige |4 oth | |
| 700 | 1 | |a Leitherer, Claus |e Sonstige |4 oth | |
| 776 | 0 | 8 | |i Erscheint auch als |n Druckausgabe |z 978-0-521-79134-2 |
| 776 | 0 | 8 | |i Erscheint auch als |n Druckausgabe |z 978-1-107-40773-2 |
| 856 | 4 | 0 | |u https://doi.org/10.1017/CBO9780511536199 |x Verlag |z URL des Erstveröffentlichers |3 Volltext |
| 912 | |a ZDB-20-CBO | ||
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| 966 | e | |u https://doi.org/10.1017/CBO9780511536199 |l FHN01 |p ZDB-20-CBO |q FHN_PDA_CBO |x Verlag |3 Volltext | |
Datensatz im Suchindex
| _version_ | 1804176885023768576 |
|---|---|
| any_adam_object | |
| author | Conti, P. S. |
| author_facet | Conti, P. S. |
| author_role | aut |
| author_sort | Conti, P. S. |
| author_variant | p s c ps psc |
| building | Verbundindex |
| bvnumber | BV043942345 |
| classification_rvk | US 4000 |
| collection | ZDB-20-CBO |
| contents | Motivation Observed properties Stellar atmospheres Stellar winds Evolution of single stars Binaries Birth of massive stars and star clusters The interstellar environment From GHII regions to starburst galaxies Starburst phenomena Cosmological implications Apparent and absolute magnitudes Distances Massive stars in Local Group galaxies Spectral classification Observations of rotation and magnetic fields LTE atmospheres Non-LTE atmospheres Surface gravities and masses Surface composition Radiation pressure Wind velocities Mass-loss rates Structure and clumping Influence of stellar rotation Nucleosynthesis Evolution to a red supergiant Evolution to the Wolf-Rayet stage Rotation and mass-loss Magnetic massive stars Core-collapse supernovae Massive binary frequency Binary masses Close binary evolution Interacting stellar winds Dust formation in WC stars Natal precursors of OB stars The initial mass function Formation of high-mass stars Massive stellar clusters Interstellar dust Ionized hydrogen regions Wind blown bubbles Ejecta nebulae around LBVs and W-R stars From giant HII regions to HII galaxies Giant HII regions: definition and structural parameters 30 Doradus -- the Rosetta Stone Stellar population diagnostics HII galaxies: stellar content and relation to starbursts Definition of a starburst The starburst IMF The evolution of starbursts Starburst-driven superwinds The starburst-AGN connection Population III stars Lyman-break galaxies Massive stars and cosmic abundances Gamma ray bursts |
| ctrlnum | (ZDB-20-CBO)CR9780511536199 (OCoLC)850916865 (DE-599)BVBBV043942345 |
| dewey-full | 523.1/125 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.1/125 |
| dewey-search | 523.1/125 |
| dewey-sort | 3523.1 3125 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1017/CBO9780511536199 |
| format | Electronic eBook |
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code="g">8.2</subfield><subfield code="g">184 --</subfield><subfield code="g">8.3</subfield><subfield code="g">187 --</subfield></datafield><datafield tag="505" ind1="8" ind2="0"><subfield code="t">Ejecta nebulae around LBVs and W-R stars</subfield><subfield code="t">From giant HII regions to HII galaxies</subfield><subfield code="t">Giant HII regions: definition and structural parameters</subfield><subfield code="t">30 Doradus -- the Rosetta Stone</subfield><subfield code="t">Stellar population diagnostics</subfield><subfield code="t">HII galaxies: stellar content and relation to starbursts</subfield><subfield code="t">Starburst phenomena</subfield><subfield code="t">Definition of a starburst</subfield><subfield code="t">The starburst IMF</subfield><subfield code="t">The evolution of starbursts</subfield><subfield code="t">Starburst-driven superwinds</subfield><subfield code="t">The starburst-AGN connection</subfield><subfield code="t">Cosmological implications</subfield><subfield code="t">Population III stars</subfield><subfield code="t">Lyman-break galaxies</subfield><subfield code="t">Massive stars and cosmic abundances</subfield><subfield code="t">Gamma ray bursts</subfield><subfield code="9"> </subfield><subfield code="g">8.4</subfield><subfield code="g">192 --</subfield><subfield code="g">9</subfield><subfield code="g">197 --</subfield><subfield code="g">9.1</subfield><subfield code="g">197 --</subfield><subfield code="g">9.2</subfield><subfield code="g">200 --</subfield><subfield code="g">9.3</subfield><subfield code="g">208 --</subfield><subfield code="g">9.4</subfield><subfield code="g">219 --</subfield><subfield code="g">10</subfield><subfield code="g">229 --</subfield><subfield code="g">10.1</subfield><subfield code="g">229 --</subfield><subfield code="g">10.2</subfield><subfield code="g">231 --</subfield><subfield code="g">10.3</subfield><subfield code="g">241 --</subfield><subfield code="g">10.4</subfield><subfield code="g">250 --</subfield><subfield code="g">10.5</subfield><subfield code="g">255 --</subfield><subfield code="g">11</subfield><subfield code="g">266 --</subfield><subfield code="g">11.1</subfield><subfield code="g">266 --</subfield><subfield code="g">11.2</subfield><subfield code="g">272 --</subfield><subfield code="g">11.3</subfield><subfield code="g">280 --</subfield><subfield code="g">11.4</subfield><subfield code="g">287</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their lives of a few million years with prodigious outputs of radiation and stellar winds, dramatically affecting both their evolution and environments. A detailed introduction to the topic, this book connects the astrophysics of massive stars with the extremes of galaxy evolution represented by starburst phenomena. A thorough discussion of the physical and wind parameters of massive stars is presented. HII galaxies, their connection to starburst galaxies, and the contribution of starburst phenomena to galaxy evolution through superwinds, are explored. The book concludes with the wider cosmological implications, including Population III stars, Lyman break galaxies and gamma-ray bursts, for each of which massive stars are believed to play a crucial role. 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| id | DE-604.BV043942345 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T07:39:17Z |
| institution | BVB |
| isbn | 9780511536199 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-029351315 |
| oclc_num | 850916865 |
| open_access_boolean | |
| owner | DE-12 DE-92 |
| owner_facet | DE-12 DE-92 |
| physical | 1 online resource (xiii, 315 pages) |
| psigel | ZDB-20-CBO ZDB-20-CBO BSB_PDA_CBO ZDB-20-CBO FHN_PDA_CBO |
| publishDate | 2008 |
| publishDateSearch | 2008 |
| publishDateSort | 2008 |
| publisher | Cambridge University Press |
| record_format | marc |
| series2 | Cambridge astrophysics |
| spelling | Conti, P. S. Verfasser aut From luminous hot stars to starburst galaxies Peter S. Conti, Paul A. Crowther, Claus Leitherer Cambridge Cambridge University Press 2008 1 online resource (xiii, 315 pages) txt rdacontent c rdamedia cr rdacarrier Cambridge astrophysics 45 Title from publisher's bibliographic system (viewed on 05 Oct 2015) 1.1 1 Motivation 1.2 1 Observed properties 1.3 5 Stellar atmospheres 1.4 5 Stellar winds 1.5 7 Evolution of single stars 1.6 9 Binaries 1.7 10 Birth of massive stars and star clusters 1.8 11 The interstellar environment 1.9 12 From GHII regions to starburst galaxies 1.10 14 Starburst phenomena 1.11 15 Cosmological implications 2 17 Observed properties 2.1 17 Apparent and absolute magnitudes 2.2 19 Distances 2.3 21 Massive stars in Local Group galaxies 2.4 35 Spectral classification 2.5 45 Observations of rotation and magnetic fields 3 49 Stellar atmospheres 3.1 49 LTE atmospheres 3.2 50 Non-LTE atmospheres 3.3 61 Surface gravities and masses 3.4 62 Surface composition 4 67 Stellar winds 4.1 67 Radiation pressure 4.2 74 Wind velocities 4.3 Mass-loss rates Structure and clumping Influence of stellar rotation Evolution of single stars Nucleosynthesis Evolution to a red supergiant Evolution to the Wolf-Rayet stage Rotation and mass-loss Magnetic massive stars Core-collapse supernovae Binaries Massive binary frequency Binary masses Close binary evolution Interacting stellar winds Dust formation in WC stars Birth of massive stars and star clusters Natal precursors of OB stars The initial mass function Formation of high-mass stars Massive stellar clusters The interstellar environment Interstellar dust Ionized hydrogen regions Wind blown bubbles 79 -- 4.4 90 -- 4.5 95 -- 5 99 -- 5.1 99 -- 5.2 102 -- 5.3 107 -- 5.4 111 -- 5.5 115 -- 5.6 116 -- 6 129 -- 6.1 129 -- 6.2 130 -- 6.3 133 -- 6.4 146 -- 6.5 149 -- 7 154 -- 7.1 155 -- 7.2 163 -- 7.3 167 -- 7.4 170 -- 8 180 -- 8.1 180 -- 8.2 184 -- 8.3 187 -- Ejecta nebulae around LBVs and W-R stars From giant HII regions to HII galaxies Giant HII regions: definition and structural parameters 30 Doradus -- the Rosetta Stone Stellar population diagnostics HII galaxies: stellar content and relation to starbursts Starburst phenomena Definition of a starburst The starburst IMF The evolution of starbursts Starburst-driven superwinds The starburst-AGN connection Cosmological implications Population III stars Lyman-break galaxies Massive stars and cosmic abundances Gamma ray bursts 8.4 192 -- 9 197 -- 9.1 197 -- 9.2 200 -- 9.3 208 -- 9.4 219 -- 10 229 -- 10.1 229 -- 10.2 231 -- 10.3 241 -- 10.4 250 -- 10.5 255 -- 11 266 -- 11.1 266 -- 11.2 272 -- 11.3 280 -- 11.4 287 Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their lives of a few million years with prodigious outputs of radiation and stellar winds, dramatically affecting both their evolution and environments. A detailed introduction to the topic, this book connects the astrophysics of massive stars with the extremes of galaxy evolution represented by starburst phenomena. A thorough discussion of the physical and wind parameters of massive stars is presented. HII galaxies, their connection to starburst galaxies, and the contribution of starburst phenomena to galaxy evolution through superwinds, are explored. The book concludes with the wider cosmological implications, including Population III stars, Lyman break galaxies and gamma-ray bursts, for each of which massive stars are believed to play a crucial role. This book is ideal for graduate students and researchers in astrophysics interested in luminous hot stars and galaxy evolution Starbursts Gamma ray bursts Stars / Evolution Stellar winds Sternwind (DE-588)4244849-9 gnd rswk-swf Starburst-Galaxie (DE-588)4298848-2 gnd rswk-swf Sternentwicklung (DE-588)4057365-5 gnd rswk-swf Sternentwicklung (DE-588)4057365-5 s Sternwind (DE-588)4244849-9 s Starburst-Galaxie (DE-588)4298848-2 s 1\p DE-604 Crowther, Paul A. Sonstige oth Leitherer, Claus Sonstige oth Erscheint auch als Druckausgabe 978-0-521-79134-2 Erscheint auch als Druckausgabe 978-1-107-40773-2 https://doi.org/10.1017/CBO9780511536199 Verlag URL des Erstveröffentlichers Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Conti, P. S. From luminous hot stars to starburst galaxies Motivation Observed properties Stellar atmospheres Stellar winds Evolution of single stars Binaries Birth of massive stars and star clusters The interstellar environment From GHII regions to starburst galaxies Starburst phenomena Cosmological implications Apparent and absolute magnitudes Distances Massive stars in Local Group galaxies Spectral classification Observations of rotation and magnetic fields LTE atmospheres Non-LTE atmospheres Surface gravities and masses Surface composition Radiation pressure Wind velocities Mass-loss rates Structure and clumping Influence of stellar rotation Nucleosynthesis Evolution to a red supergiant Evolution to the Wolf-Rayet stage Rotation and mass-loss Magnetic massive stars Core-collapse supernovae Massive binary frequency Binary masses Close binary evolution Interacting stellar winds Dust formation in WC stars Natal precursors of OB stars The initial mass function Formation of high-mass stars Massive stellar clusters Interstellar dust Ionized hydrogen regions Wind blown bubbles Ejecta nebulae around LBVs and W-R stars From giant HII regions to HII galaxies Giant HII regions: definition and structural parameters 30 Doradus -- the Rosetta Stone Stellar population diagnostics HII galaxies: stellar content and relation to starbursts Definition of a starburst The starburst IMF The evolution of starbursts Starburst-driven superwinds The starburst-AGN connection Population III stars Lyman-break galaxies Massive stars and cosmic abundances Gamma ray bursts Starbursts Gamma ray bursts Stars / Evolution Stellar winds Sternwind (DE-588)4244849-9 gnd Starburst-Galaxie (DE-588)4298848-2 gnd Sternentwicklung (DE-588)4057365-5 gnd |
| subject_GND | (DE-588)4244849-9 (DE-588)4298848-2 (DE-588)4057365-5 |
| title | From luminous hot stars to starburst galaxies |
| title_alt | Motivation Observed properties Stellar atmospheres Stellar winds Evolution of single stars Binaries Birth of massive stars and star clusters The interstellar environment From GHII regions to starburst galaxies Starburst phenomena Cosmological implications Apparent and absolute magnitudes Distances Massive stars in Local Group galaxies Spectral classification Observations of rotation and magnetic fields LTE atmospheres Non-LTE atmospheres Surface gravities and masses Surface composition Radiation pressure Wind velocities Mass-loss rates Structure and clumping Influence of stellar rotation Nucleosynthesis Evolution to a red supergiant Evolution to the Wolf-Rayet stage Rotation and mass-loss Magnetic massive stars Core-collapse supernovae Massive binary frequency Binary masses Close binary evolution Interacting stellar winds Dust formation in WC stars Natal precursors of OB stars The initial mass function Formation of high-mass stars Massive stellar clusters Interstellar dust Ionized hydrogen regions Wind blown bubbles Ejecta nebulae around LBVs and W-R stars From giant HII regions to HII galaxies Giant HII regions: definition and structural parameters 30 Doradus -- the Rosetta Stone Stellar population diagnostics HII galaxies: stellar content and relation to starbursts Definition of a starburst The starburst IMF The evolution of starbursts Starburst-driven superwinds The starburst-AGN connection Population III stars Lyman-break galaxies Massive stars and cosmic abundances Gamma ray bursts |
| title_auth | From luminous hot stars to starburst galaxies |
| title_exact_search | From luminous hot stars to starburst galaxies |
| title_full | From luminous hot stars to starburst galaxies Peter S. Conti, Paul A. Crowther, Claus Leitherer |
| title_fullStr | From luminous hot stars to starburst galaxies Peter S. Conti, Paul A. Crowther, Claus Leitherer |
| title_full_unstemmed | From luminous hot stars to starburst galaxies Peter S. Conti, Paul A. Crowther, Claus Leitherer |
| title_short | From luminous hot stars to starburst galaxies |
| title_sort | from luminous hot stars to starburst galaxies |
| topic | Starbursts Gamma ray bursts Stars / Evolution Stellar winds Sternwind (DE-588)4244849-9 gnd Starburst-Galaxie (DE-588)4298848-2 gnd Sternentwicklung (DE-588)4057365-5 gnd |
| topic_facet | Starbursts Gamma ray bursts Stars / Evolution Stellar winds Sternwind Starburst-Galaxie Sternentwicklung |
| url | https://doi.org/10.1017/CBO9780511536199 |
| work_keys_str_mv | AT contips fromluminoushotstarstostarburstgalaxies AT crowtherpaula fromluminoushotstarstostarburstgalaxies AT leithererclaus fromluminoushotstarstostarburstgalaxies |