PRECISE MEASUREMENT OF STELLAR TEMPERATURES USING LINE-DEPTH RATIOS
The ratio of line depth for two spectral lines is used to determine stellar temperatures with a precision = 10 K = 0.2 percent. For stars between late-F and early-K spectral types, the V I 6251 to Fe I 6253 depth ratio is easy to measure. It is also applicable to other temperature regimes if suitabl...
Gespeichert in:
Veröffentlicht in: | Publications of the Astronomical Society of the Pacific 1991-05, Vol.103 (663), p.439-443 |
---|---|
Hauptverfasser: | , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 443 |
---|---|
container_issue | 663 |
container_start_page | 439 |
container_title | Publications of the Astronomical Society of the Pacific |
container_volume | 103 |
creator | GRAY, DAVID F. JOHANSON, HEATHER L. |
description | The ratio of line depth for two spectral lines is used to determine stellar temperatures with a precision = 10 K = 0.2 percent. For stars between late-F and early-K spectral types, the V I 6251 to Fe I 6253 depth ratio is easy to measure. It is also applicable to other temperature regimes if suitable lines can be found. 14 refs. |
doi_str_mv | 10.1086/132839 |
format | Article |
fullrecord | <record><control><sourceid>jstor_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_5588551</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><jstor_id>40679707</jstor_id><sourcerecordid>40679707</sourcerecordid><originalsourceid>FETCH-LOGICAL-c300t-32b59f19923e88aaaa816ba816032ad6d24b01ea3ac757a081c5b10aa56360ce3</originalsourceid><addsrcrecordid>eNo90D1PwzAQBmALgUQp8A-QLAa2wF2udpwxCm4bKf1Qks6R47qiFTQozsK_J1UQN9wN76MbXsYeEV4RlHxDChXFV2yCglRAKqJrNgGAWSBDBbfszvsTAKJCmLB0W-g0KzVf6aTcFXql1xXfzHlZ6TxPCl7p1VYXSTVEJd-V2XrB82ytg3e9rZZ8CLJNec9uDubTu4e_O2W7ua7SZZBvFlma5IElgD6gsBHxAeM4JKeUGUahbC4LKDR7uQ9nDaAzZGwkIgMKrWgQjBGSJFhHU_Y8_m19f6y9PfbOftj2fHa2r4VQSggc0MuIbNd637lD_d0dv0z3UyPUl37qsZ8BPo3w5Pu2-1czkFEcQUS_QoxZOg</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>PRECISE MEASUREMENT OF STELLAR TEMPERATURES USING LINE-DEPTH RATIOS</title><source>Jstor Complete Legacy</source><source>IOP Publishing Journals</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>Institute of Physics (IOP) Journals - HEAL-Link</source><source>Alma/SFX Local Collection</source><creator>GRAY, DAVID F. ; JOHANSON, HEATHER L.</creator><creatorcontrib>GRAY, DAVID F. ; JOHANSON, HEATHER L.</creatorcontrib><description>The ratio of line depth for two spectral lines is used to determine stellar temperatures with a precision = 10 K = 0.2 percent. For stars between late-F and early-K spectral types, the V I 6251 to Fe I 6253 depth ratio is easy to measure. It is also applicable to other temperature regimes if suitable lines can be found. 14 refs.</description><identifier>ISSN: 0004-6280</identifier><identifier>EISSN: 1538-3873</identifier><identifier>DOI: 10.1086/132839</identifier><language>eng</language><publisher>United States: The Astronomical Society of the Pacific</publisher><subject>640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources ; ACCURACY ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; DWARF STARS ; Effective temperature ; Error rates ; LUMINOSITY ; OPTICAL PROPERTIES ; PHYSICAL PROPERTIES ; Polynomials ; SPECTRA ; STARS ; Stellar classification ; Stellar spectra ; Stellar temperature ; Temperature gradients ; TEMPERATURE MEASUREMENT ; Temperature ratio</subject><ispartof>Publications of the Astronomical Society of the Pacific, 1991-05, Vol.103 (663), p.439-443</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c300t-32b59f19923e88aaaa816ba816032ad6d24b01ea3ac757a081c5b10aa56360ce3</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/40679707$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/40679707$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>230,314,776,780,799,881,27901,27902,57992,58225</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/5588551$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>GRAY, DAVID F.</creatorcontrib><creatorcontrib>JOHANSON, HEATHER L.</creatorcontrib><title>PRECISE MEASUREMENT OF STELLAR TEMPERATURES USING LINE-DEPTH RATIOS</title><title>Publications of the Astronomical Society of the Pacific</title><description>The ratio of line depth for two spectral lines is used to determine stellar temperatures with a precision = 10 K = 0.2 percent. For stars between late-F and early-K spectral types, the V I 6251 to Fe I 6253 depth ratio is easy to measure. It is also applicable to other temperature regimes if suitable lines can be found. 14 refs.</description><subject>640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources</subject><subject>ACCURACY</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>DWARF STARS</subject><subject>Effective temperature</subject><subject>Error rates</subject><subject>LUMINOSITY</subject><subject>OPTICAL PROPERTIES</subject><subject>PHYSICAL PROPERTIES</subject><subject>Polynomials</subject><subject>SPECTRA</subject><subject>STARS</subject><subject>Stellar classification</subject><subject>Stellar spectra</subject><subject>Stellar temperature</subject><subject>Temperature gradients</subject><subject>TEMPERATURE MEASUREMENT</subject><subject>Temperature ratio</subject><issn>0004-6280</issn><issn>1538-3873</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1991</creationdate><recordtype>article</recordtype><recordid>eNo90D1PwzAQBmALgUQp8A-QLAa2wF2udpwxCm4bKf1Qks6R47qiFTQozsK_J1UQN9wN76MbXsYeEV4RlHxDChXFV2yCglRAKqJrNgGAWSBDBbfszvsTAKJCmLB0W-g0KzVf6aTcFXql1xXfzHlZ6TxPCl7p1VYXSTVEJd-V2XrB82ytg3e9rZZ8CLJNec9uDubTu4e_O2W7ua7SZZBvFlma5IElgD6gsBHxAeM4JKeUGUahbC4LKDR7uQ9nDaAzZGwkIgMKrWgQjBGSJFhHU_Y8_m19f6y9PfbOftj2fHa2r4VQSggc0MuIbNd637lD_d0dv0z3UyPUl37qsZ8BPo3w5Pu2-1czkFEcQUS_QoxZOg</recordid><startdate>19910501</startdate><enddate>19910501</enddate><creator>GRAY, DAVID F.</creator><creator>JOHANSON, HEATHER L.</creator><general>The Astronomical Society of the Pacific</general><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope></search><sort><creationdate>19910501</creationdate><title>PRECISE MEASUREMENT OF STELLAR TEMPERATURES USING LINE-DEPTH RATIOS</title><author>GRAY, DAVID F. ; JOHANSON, HEATHER L.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c300t-32b59f19923e88aaaa816ba816032ad6d24b01ea3ac757a081c5b10aa56360ce3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1991</creationdate><topic>640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources</topic><topic>ACCURACY</topic><topic>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</topic><topic>DWARF STARS</topic><topic>Effective temperature</topic><topic>Error rates</topic><topic>LUMINOSITY</topic><topic>OPTICAL PROPERTIES</topic><topic>PHYSICAL PROPERTIES</topic><topic>Polynomials</topic><topic>SPECTRA</topic><topic>STARS</topic><topic>Stellar classification</topic><topic>Stellar spectra</topic><topic>Stellar temperature</topic><topic>Temperature gradients</topic><topic>TEMPERATURE MEASUREMENT</topic><topic>Temperature ratio</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>GRAY, DAVID F.</creatorcontrib><creatorcontrib>JOHANSON, HEATHER L.</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Publications of the Astronomical Society of the Pacific</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>GRAY, DAVID F.</au><au>JOHANSON, HEATHER L.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>PRECISE MEASUREMENT OF STELLAR TEMPERATURES USING LINE-DEPTH RATIOS</atitle><jtitle>Publications of the Astronomical Society of the Pacific</jtitle><date>1991-05-01</date><risdate>1991</risdate><volume>103</volume><issue>663</issue><spage>439</spage><epage>443</epage><pages>439-443</pages><issn>0004-6280</issn><eissn>1538-3873</eissn><abstract>The ratio of line depth for two spectral lines is used to determine stellar temperatures with a precision = 10 K = 0.2 percent. For stars between late-F and early-K spectral types, the V I 6251 to Fe I 6253 depth ratio is easy to measure. It is also applicable to other temperature regimes if suitable lines can be found. 14 refs.</abstract><cop>United States</cop><pub>The Astronomical Society of the Pacific</pub><doi>10.1086/132839</doi><tpages>5</tpages><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0004-6280 |
ispartof | Publications of the Astronomical Society of the Pacific, 1991-05, Vol.103 (663), p.439-443 |
issn | 0004-6280 1538-3873 |
language | eng |
recordid | cdi_osti_scitechconnect_5588551 |
source | Jstor Complete Legacy; IOP Publishing Journals; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Institute of Physics (IOP) Journals - HEAL-Link; Alma/SFX Local Collection |
subjects | 640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources ACCURACY CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS DWARF STARS Effective temperature Error rates LUMINOSITY OPTICAL PROPERTIES PHYSICAL PROPERTIES Polynomials SPECTRA STARS Stellar classification Stellar spectra Stellar temperature Temperature gradients TEMPERATURE MEASUREMENT Temperature ratio |
title | PRECISE MEASUREMENT OF STELLAR TEMPERATURES USING LINE-DEPTH RATIOS |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-21T18%3A51%3A23IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-jstor_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=PRECISE%20MEASUREMENT%20OF%20STELLAR%20TEMPERATURES%20USING%20LINE-DEPTH%20RATIOS&rft.jtitle=Publications%20of%20the%20Astronomical%20Society%20of%20the%20Pacific&rft.au=GRAY,%20DAVID%20F.&rft.date=1991-05-01&rft.volume=103&rft.issue=663&rft.spage=439&rft.epage=443&rft.pages=439-443&rft.issn=0004-6280&rft.eissn=1538-3873&rft_id=info:doi/10.1086/132839&rft_dat=%3Cjstor_osti_%3E40679707%3C/jstor_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/&rft_jstor_id=40679707&rfr_iscdi=true |