Bolometric-Correction and Effective-Temperature Scale
IN recent years the application of high-speed digital computers to problems in theoretical astrophysics has combined with fundamental research in nuclear physics and solar convection to achieve considerable understanding of the physics of not only stellar interiors but also stellar evolution. The co...
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| Veröffentlicht in: | Nature (London) 1963-09, Vol.199 (4897), p.988-990 |
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| container_title | Nature (London) |
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| creator | WILDEY, ROBERT L |
| description | IN recent years the application of high-speed digital computers to problems in theoretical astrophysics has combined with fundamental research in nuclear physics and solar convection to achieve considerable understanding of the physics of not only stellar interiors but also stellar evolution. The connecting link between this increasingly elaborate theory and the corresponding ensemble of observations is the scale of bolometric-corrections (
B.C.
) and effective-temperatures (
Te
). |
| doi_str_mv | 10.1038/199988a0 |
| format | Article |
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B.C.
) and effective-temperatures (
Te
).</description><identifier>ISSN: 0028-0836</identifier><identifier>EISSN: 1476-4687</identifier><identifier>DOI: 10.1038/199988a0</identifier><language>eng</language><publisher>London: Nature Publishing Group UK</publisher><subject>ASTRONOMY AND ASTROPHYSICS ; ASTROPHYSICS ; COMPUTERS ; HIGH TEMPERATURE ; Humanities and Social Sciences ; letter ; multidisciplinary ; NUCLEAR REACTIONS ; QUANTITATIVE ANALYSIS ; Science ; Science (multidisciplinary) ; STARS ; SUN</subject><ispartof>Nature (London), 1963-09, Vol.199 (4897), p.988-990</ispartof><rights>Springer Nature Limited 1963</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c309t-7fde393e3026fed07253d38edae3972cd827ac684e583c9c3f2f30b09f4c611c3</citedby><cites>FETCH-LOGICAL-c309t-7fde393e3026fed07253d38edae3972cd827ac684e583c9c3f2f30b09f4c611c3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1038/199988a0$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1038/199988a0$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>230,314,780,784,885,2726,27923,27924,41487,42556,51318</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/4635709$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>WILDEY, ROBERT L</creatorcontrib><creatorcontrib>Carnegie Institution of Washington, D.C</creatorcontrib><creatorcontrib>California Inst. of Tech., Pasadena</creatorcontrib><title>Bolometric-Correction and Effective-Temperature Scale</title><title>Nature (London)</title><addtitle>Nature</addtitle><description>IN recent years the application of high-speed digital computers to problems in theoretical astrophysics has combined with fundamental research in nuclear physics and solar convection to achieve considerable understanding of the physics of not only stellar interiors but also stellar evolution. The connecting link between this increasingly elaborate theory and the corresponding ensemble of observations is the scale of bolometric-corrections (
B.C.
) and effective-temperatures (
Te
).</description><subject>ASTRONOMY AND ASTROPHYSICS</subject><subject>ASTROPHYSICS</subject><subject>COMPUTERS</subject><subject>HIGH TEMPERATURE</subject><subject>Humanities and Social Sciences</subject><subject>letter</subject><subject>multidisciplinary</subject><subject>NUCLEAR REACTIONS</subject><subject>QUANTITATIVE ANALYSIS</subject><subject>Science</subject><subject>Science (multidisciplinary)</subject><subject>STARS</subject><subject>SUN</subject><issn>0028-0836</issn><issn>1476-4687</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1963</creationdate><recordtype>article</recordtype><recordid>eNpt0E1LAzEQBuAgCtYq-AukeNJDdLLZzcdRS_2AggfreYmzE93SJiXZCv57t67ixdMww8Mw8zJ2KuBKgDTXwlprjIM9NhKlVrxURu-zEUBhOBipDtlRzksAqIQuR6y6jau4pi61yKcxJcKujWHiQjOZeb_rPogvaL2h5LptoskzuhUdswPvVplOfuqYvdzNFtMHPn-6f5zezDlKsB3XviFpJUkolKcGdFHJRhpqXD_WBTam0A6VKakyEi1KX3gJr2B9iUoIlGN2PuyNuWvrjG1H-I4xhP6wulSy0mB7dDEgTDHnRL7epHbt0mctoN5lUv9m0tPLgeaehDdK9TJuU-hf-M-eDTZ8P_639Bd8Afo2alc</recordid><startdate>19630907</startdate><enddate>19630907</enddate><creator>WILDEY, ROBERT L</creator><general>Nature Publishing Group UK</general><general>Nature Publishing Group</general><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope></search><sort><creationdate>19630907</creationdate><title>Bolometric-Correction and Effective-Temperature Scale</title><author>WILDEY, ROBERT L</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c309t-7fde393e3026fed07253d38edae3972cd827ac684e583c9c3f2f30b09f4c611c3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1963</creationdate><topic>ASTRONOMY AND ASTROPHYSICS</topic><topic>ASTROPHYSICS</topic><topic>COMPUTERS</topic><topic>HIGH TEMPERATURE</topic><topic>Humanities and Social Sciences</topic><topic>letter</topic><topic>multidisciplinary</topic><topic>NUCLEAR REACTIONS</topic><topic>QUANTITATIVE ANALYSIS</topic><topic>Science</topic><topic>Science (multidisciplinary)</topic><topic>STARS</topic><topic>SUN</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>WILDEY, ROBERT L</creatorcontrib><creatorcontrib>Carnegie Institution of Washington, D.C</creatorcontrib><creatorcontrib>California Inst. of Tech., Pasadena</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Nature (London)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>WILDEY, ROBERT L</au><aucorp>Carnegie Institution of Washington, D.C</aucorp><aucorp>California Inst. of Tech., Pasadena</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Bolometric-Correction and Effective-Temperature Scale</atitle><jtitle>Nature (London)</jtitle><stitle>Nature</stitle><date>1963-09-07</date><risdate>1963</risdate><volume>199</volume><issue>4897</issue><spage>988</spage><epage>990</epage><pages>988-990</pages><issn>0028-0836</issn><eissn>1476-4687</eissn><abstract>IN recent years the application of high-speed digital computers to problems in theoretical astrophysics has combined with fundamental research in nuclear physics and solar convection to achieve considerable understanding of the physics of not only stellar interiors but also stellar evolution. The connecting link between this increasingly elaborate theory and the corresponding ensemble of observations is the scale of bolometric-corrections (
B.C.
) and effective-temperatures (
Te
).</abstract><cop>London</cop><pub>Nature Publishing Group UK</pub><doi>10.1038/199988a0</doi><tpages>3</tpages></addata></record> |
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| ispartof | Nature (London), 1963-09, Vol.199 (4897), p.988-990 |
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| language | eng |
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| subjects | ASTRONOMY AND ASTROPHYSICS ASTROPHYSICS COMPUTERS HIGH TEMPERATURE Humanities and Social Sciences letter multidisciplinary NUCLEAR REACTIONS QUANTITATIVE ANALYSIS Science Science (multidisciplinary) STARS SUN |
| title | Bolometric-Correction and Effective-Temperature Scale |
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