Stellar winds and the evolution of luminous stars
The effect of a stellar wind on the evolution of stars in the mass range 7--60 M/sub sun/ has been investigated for stellar models in which Carson's opacities have been employed. Several cases of mass loss have been considered. It is found that the assumption of heavy mass loss from both blue a...
Gespeichert in:
| Veröffentlicht in: | Astrophys. J.; (United States) 1978-11, Vol.226, p.231 |
|---|---|
| Hauptverfasser: | , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | |
| container_start_page | 231 |
| container_title | Astrophys. J.; (United States) |
| container_volume | 226 |
| creator | Stothers, R. Chin, C.-W. |
| description | The effect of a stellar wind on the evolution of stars in the mass range 7--60 M/sub sun/ has been investigated for stellar models in which Carson's opacities have been employed. Several cases of mass loss have been considered. It is found that the assumption of heavy mass loss from both blue and red supergiants can account well for the relevant observations of OBN stars, WN stars, and very luminous supergiants of all spectral types. But no amount of mass loss can account adequately for the properties of the B supergiants of lowest luminosity. A critical comparison is made between the present results and some earlier results based on the adoption of Cox-Stewart opacities. |
| doi_str_mv | 10.1086/156602 |
| format | Article |
| fullrecord | <record><control><sourceid>crossref_osti_</sourceid><recordid>TN_cdi_crossref_primary_10_1086_156602</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>10_1086_156602</sourcerecordid><originalsourceid>FETCH-LOGICAL-c180t-d52f8939a3a4b293162a06544737dec2407d18f5191f11b8297bf34083633c113</originalsourceid><addsrcrecordid>eNotkE1LxDAURYMoWEf9DcGFu2peXpImSxn8ggEXKrgraZowlU4jSar4752hri4XDhfuIeQS2A0wrW5BKsX4EalAoq4FyuaYVIwxUStsPk7JWc6fh8qNqQi8Fj-ONtGfYeoztVNPy9ZT_x3HuQxxojHQcd4NU5wzzcWmfE5Ogh2zv_jPFXl_uH9bP9Wbl8fn9d2mdqBZqXvJgzZoLFrRcYOguGVKCtFg03vHBWt60EGCgQDQaW6aLqBgGhWiA8AVuVp2Yy5Dm91QvNu6OE3elVZJbfYv99D1ArkUc04-tF9p2Nn02wJrDzbaxQb-AfkoToA</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Stellar winds and the evolution of luminous stars</title><source>Alma/SFX Local Collection</source><creator>Stothers, R. ; Chin, C.-W.</creator><creatorcontrib>Stothers, R. ; Chin, C.-W. ; NASA Goddard Institute fro Space Studeis, Goddard Space Flight Center, New York</creatorcontrib><description>The effect of a stellar wind on the evolution of stars in the mass range 7--60 M/sub sun/ has been investigated for stellar models in which Carson's opacities have been employed. Several cases of mass loss have been considered. It is found that the assumption of heavy mass loss from both blue and red supergiants can account well for the relevant observations of OBN stars, WN stars, and very luminous supergiants of all spectral types. But no amount of mass loss can account adequately for the properties of the B supergiants of lowest luminosity. A critical comparison is made between the present results and some earlier results based on the adoption of Cox-Stewart opacities.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1086/156602</identifier><language>eng</language><publisher>United States</publisher><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; DIAGRAMS ; GIANT STARS ; HERTZSPRUNG-RUSSELL DIAGRAM ; MATHEMATICAL MODELS ; NUCLEOSYNTHESIS ; STAR EVOLUTION ; STAR MODELS ; STARS 640102 -- Astrophysics & Cosmology-- Stars & Quasi-Stellar, Radio & X-Ray Sources ; STELLAR WINDS ; SUPERGIANT STARS</subject><ispartof>Astrophys. J.; (United States), 1978-11, Vol.226, p.231</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c180t-d52f8939a3a4b293162a06544737dec2407d18f5191f11b8297bf34083633c113</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,885,27924,27925</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/6589660$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Stothers, R.</creatorcontrib><creatorcontrib>Chin, C.-W.</creatorcontrib><creatorcontrib>NASA Goddard Institute fro Space Studeis, Goddard Space Flight Center, New York</creatorcontrib><title>Stellar winds and the evolution of luminous stars</title><title>Astrophys. J.; (United States)</title><description>The effect of a stellar wind on the evolution of stars in the mass range 7--60 M/sub sun/ has been investigated for stellar models in which Carson's opacities have been employed. Several cases of mass loss have been considered. It is found that the assumption of heavy mass loss from both blue and red supergiants can account well for the relevant observations of OBN stars, WN stars, and very luminous supergiants of all spectral types. But no amount of mass loss can account adequately for the properties of the B supergiants of lowest luminosity. A critical comparison is made between the present results and some earlier results based on the adoption of Cox-Stewart opacities.</description><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>DIAGRAMS</subject><subject>GIANT STARS</subject><subject>HERTZSPRUNG-RUSSELL DIAGRAM</subject><subject>MATHEMATICAL MODELS</subject><subject>NUCLEOSYNTHESIS</subject><subject>STAR EVOLUTION</subject><subject>STAR MODELS</subject><subject>STARS 640102 -- Astrophysics & Cosmology-- Stars & Quasi-Stellar, Radio & X-Ray Sources</subject><subject>STELLAR WINDS</subject><subject>SUPERGIANT STARS</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1978</creationdate><recordtype>article</recordtype><recordid>eNotkE1LxDAURYMoWEf9DcGFu2peXpImSxn8ggEXKrgraZowlU4jSar4752hri4XDhfuIeQS2A0wrW5BKsX4EalAoq4FyuaYVIwxUStsPk7JWc6fh8qNqQi8Fj-ONtGfYeoztVNPy9ZT_x3HuQxxojHQcd4NU5wzzcWmfE5Ogh2zv_jPFXl_uH9bP9Wbl8fn9d2mdqBZqXvJgzZoLFrRcYOguGVKCtFg03vHBWt60EGCgQDQaW6aLqBgGhWiA8AVuVp2Yy5Dm91QvNu6OE3elVZJbfYv99D1ArkUc04-tF9p2Nn02wJrDzbaxQb-AfkoToA</recordid><startdate>19781115</startdate><enddate>19781115</enddate><creator>Stothers, R.</creator><creator>Chin, C.-W.</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope></search><sort><creationdate>19781115</creationdate><title>Stellar winds and the evolution of luminous stars</title><author>Stothers, R. ; Chin, C.-W.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c180t-d52f8939a3a4b293162a06544737dec2407d18f5191f11b8297bf34083633c113</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1978</creationdate><topic>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</topic><topic>DIAGRAMS</topic><topic>GIANT STARS</topic><topic>HERTZSPRUNG-RUSSELL DIAGRAM</topic><topic>MATHEMATICAL MODELS</topic><topic>NUCLEOSYNTHESIS</topic><topic>STAR EVOLUTION</topic><topic>STAR MODELS</topic><topic>STARS 640102 -- Astrophysics & Cosmology-- Stars & Quasi-Stellar, Radio & X-Ray Sources</topic><topic>STELLAR WINDS</topic><topic>SUPERGIANT STARS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Stothers, R.</creatorcontrib><creatorcontrib>Chin, C.-W.</creatorcontrib><creatorcontrib>NASA Goddard Institute fro Space Studeis, Goddard Space Flight Center, New York</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Astrophys. J.; (United States)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Stothers, R.</au><au>Chin, C.-W.</au><aucorp>NASA Goddard Institute fro Space Studeis, Goddard Space Flight Center, New York</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Stellar winds and the evolution of luminous stars</atitle><jtitle>Astrophys. J.; (United States)</jtitle><date>1978-11-15</date><risdate>1978</risdate><volume>226</volume><spage>231</spage><pages>231-</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>The effect of a stellar wind on the evolution of stars in the mass range 7--60 M/sub sun/ has been investigated for stellar models in which Carson's opacities have been employed. Several cases of mass loss have been considered. It is found that the assumption of heavy mass loss from both blue and red supergiants can account well for the relevant observations of OBN stars, WN stars, and very luminous supergiants of all spectral types. But no amount of mass loss can account adequately for the properties of the B supergiants of lowest luminosity. A critical comparison is made between the present results and some earlier results based on the adoption of Cox-Stewart opacities.</abstract><cop>United States</cop><doi>10.1086/156602</doi></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0004-637X |
| ispartof | Astrophys. J.; (United States), 1978-11, Vol.226, p.231 |
| issn | 0004-637X 1538-4357 |
| language | eng |
| recordid | cdi_crossref_primary_10_1086_156602 |
| source | Alma/SFX Local Collection |
| subjects | CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS DIAGRAMS GIANT STARS HERTZSPRUNG-RUSSELL DIAGRAM MATHEMATICAL MODELS NUCLEOSYNTHESIS STAR EVOLUTION STAR MODELS STARS 640102 -- Astrophysics & Cosmology-- Stars & Quasi-Stellar, Radio & X-Ray Sources STELLAR WINDS SUPERGIANT STARS |
| title | Stellar winds and the evolution of luminous stars |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-04T20%3A44%3A44IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-crossref_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Stellar%20winds%20and%20the%20evolution%20of%20luminous%20stars&rft.jtitle=Astrophys.%20J.;%20(United%20States)&rft.au=Stothers,%20R.&rft.aucorp=NASA%20Goddard%20Institute%20fro%20Space%20Studeis,%20Goddard%20Space%20Flight%20Center,%20New%20York&rft.date=1978-11-15&rft.volume=226&rft.spage=231&rft.pages=231-&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.1086/156602&rft_dat=%3Ccrossref_osti_%3E10_1086_156602%3C/crossref_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |