On the 1893 Absorption-Line Spectrum of Eta Carinae
It is suggested that several features present in the 1893 absorption-line spectrum of Eta Carinae may be due to high-excitation lines of neutral carbon not seen in the spectra of stars of normal chemical composition. This perhaps implies a relationship of this unique southern variable to the stars o...
Gespeichert in:
| Veröffentlicht in: | Publications of the Astronomical Society of the Pacific 1993-06, Vol.105 (688), p.578-578 |
|---|---|
| 1. Verfasser: | |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 578 |
|---|---|
| container_issue | 688 |
| container_start_page | 578 |
| container_title | Publications of the Astronomical Society of the Pacific |
| container_volume | 105 |
| creator | Bidelman, William P. |
| description | It is suggested that several features present in the 1893 absorption-line spectrum of Eta Carinae may be due to high-excitation lines of neutral carbon not seen in the spectra of stars of normal chemical composition. This perhaps implies a relationship of this unique southern variable to the stars of the R Coronae Borealis type. |
| doi_str_mv | 10.1086/133197 |
| format | Article |
| fullrecord | <record><control><sourceid>jstor_cross</sourceid><recordid>TN_cdi_crossref_primary_10_1086_133197</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><jstor_id>40680073</jstor_id><sourcerecordid>40680073</sourcerecordid><originalsourceid>FETCH-LOGICAL-c199t-51799f0f8649864982d4b4fa3e39fecb1b5827701363f6e43d7fe8c0707085eb3</originalsourceid><addsrcrecordid>eNpFj01LxDAURYMoOI76D4QsxF30vb60SZZDGT-gMAt1XdJMgh1m2pLUhf_eOhXlcXmLe7hwGLtGuEfQxQMSoVEnbIE5aUFa0SlbAIAURabhnF2ktANA1AgLRpuOjx-eozbEV03q4zC2fSeqtvP8dfBujJ8H3ge-Hi0vbWw76y_ZWbD75K9-_5K9P67fymdRbZ5eylUlHBozihyVMQGCLqQ5JtvKRgZLnkzwrsEm15lSgFRQKLykrQpeO1DT6dw3tGR3866LfUrRh3qI7cHGrxqh_lGtZ9UJvJ3BwSZn9yHazrXpj5b6KDthNzO2S2Mf_2soNIAi-gZHO1hd</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>On the 1893 Absorption-Line Spectrum of Eta Carinae</title><source>IOP Publishing Journals</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>JSTOR Archive Collection A-Z Listing</source><source>Institute of Physics (IOP) Journals - HEAL-Link</source><source>Alma/SFX Local Collection</source><creator>Bidelman, William P.</creator><creatorcontrib>Bidelman, William P.</creatorcontrib><description>It is suggested that several features present in the 1893 absorption-line spectrum of Eta Carinae may be due to high-excitation lines of neutral carbon not seen in the spectra of stars of normal chemical composition. This perhaps implies a relationship of this unique southern variable to the stars of the R Coronae Borealis type.</description><identifier>ISSN: 0004-6280</identifier><identifier>EISSN: 1538-3873</identifier><identifier>DOI: 10.1086/133197</identifier><identifier>CODEN: PASPAU</identifier><language>eng</language><publisher>Chicago, IL: American Institute of Physics</publisher><subject>Absorption spectra ; Astronomy ; Carbon ; Earth, ocean, space ; Emission spectra ; Exact sciences and technology ; Hydrogen ; Line spectra ; R Coronae Borealis variables ; Spectral bands ; Stars ; Stellar spectra ; Stellar spectral lines ; Unusual and peculiar variables ; Variable and peculiar stars (including novae)</subject><ispartof>Publications of the Astronomical Society of the Pacific, 1993-06, Vol.105 (688), p.578-578</ispartof><rights>1993 INIST-CNRS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/40680073$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/40680073$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>315,782,786,805,27931,27932,58024,58257</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=4811810$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Bidelman, William P.</creatorcontrib><title>On the 1893 Absorption-Line Spectrum of Eta Carinae</title><title>Publications of the Astronomical Society of the Pacific</title><description>It is suggested that several features present in the 1893 absorption-line spectrum of Eta Carinae may be due to high-excitation lines of neutral carbon not seen in the spectra of stars of normal chemical composition. This perhaps implies a relationship of this unique southern variable to the stars of the R Coronae Borealis type.</description><subject>Absorption spectra</subject><subject>Astronomy</subject><subject>Carbon</subject><subject>Earth, ocean, space</subject><subject>Emission spectra</subject><subject>Exact sciences and technology</subject><subject>Hydrogen</subject><subject>Line spectra</subject><subject>R Coronae Borealis variables</subject><subject>Spectral bands</subject><subject>Stars</subject><subject>Stellar spectra</subject><subject>Stellar spectral lines</subject><subject>Unusual and peculiar variables</subject><subject>Variable and peculiar stars (including novae)</subject><issn>0004-6280</issn><issn>1538-3873</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1993</creationdate><recordtype>article</recordtype><recordid>eNpFj01LxDAURYMoOI76D4QsxF30vb60SZZDGT-gMAt1XdJMgh1m2pLUhf_eOhXlcXmLe7hwGLtGuEfQxQMSoVEnbIE5aUFa0SlbAIAURabhnF2ktANA1AgLRpuOjx-eozbEV03q4zC2fSeqtvP8dfBujJ8H3ge-Hi0vbWw76y_ZWbD75K9-_5K9P67fymdRbZ5eylUlHBozihyVMQGCLqQ5JtvKRgZLnkzwrsEm15lSgFRQKLykrQpeO1DT6dw3tGR3866LfUrRh3qI7cHGrxqh_lGtZ9UJvJ3BwSZn9yHazrXpj5b6KDthNzO2S2Mf_2soNIAi-gZHO1hd</recordid><startdate>19930601</startdate><enddate>19930601</enddate><creator>Bidelman, William P.</creator><general>American Institute of Physics</general><general>University of Chicago Press</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>19930601</creationdate><title>On the 1893 Absorption-Line Spectrum of Eta Carinae</title><author>Bidelman, William P.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c199t-51799f0f8649864982d4b4fa3e39fecb1b5827701363f6e43d7fe8c0707085eb3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1993</creationdate><topic>Absorption spectra</topic><topic>Astronomy</topic><topic>Carbon</topic><topic>Earth, ocean, space</topic><topic>Emission spectra</topic><topic>Exact sciences and technology</topic><topic>Hydrogen</topic><topic>Line spectra</topic><topic>R Coronae Borealis variables</topic><topic>Spectral bands</topic><topic>Stars</topic><topic>Stellar spectra</topic><topic>Stellar spectral lines</topic><topic>Unusual and peculiar variables</topic><topic>Variable and peculiar stars (including novae)</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Bidelman, William P.</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><jtitle>Publications of the Astronomical Society of the Pacific</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Bidelman, William P.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>On the 1893 Absorption-Line Spectrum of Eta Carinae</atitle><jtitle>Publications of the Astronomical Society of the Pacific</jtitle><date>1993-06-01</date><risdate>1993</risdate><volume>105</volume><issue>688</issue><spage>578</spage><epage>578</epage><pages>578-578</pages><issn>0004-6280</issn><eissn>1538-3873</eissn><coden>PASPAU</coden><abstract>It is suggested that several features present in the 1893 absorption-line spectrum of Eta Carinae may be due to high-excitation lines of neutral carbon not seen in the spectra of stars of normal chemical composition. This perhaps implies a relationship of this unique southern variable to the stars of the R Coronae Borealis type.</abstract><cop>Chicago, IL</cop><pub>American Institute of Physics</pub><doi>10.1086/133197</doi><tpages>1</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0004-6280 |
| ispartof | Publications of the Astronomical Society of the Pacific, 1993-06, Vol.105 (688), p.578-578 |
| issn | 0004-6280 1538-3873 |
| language | eng |
| recordid | cdi_crossref_primary_10_1086_133197 |
| source | IOP Publishing Journals; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; JSTOR Archive Collection A-Z Listing; Institute of Physics (IOP) Journals - HEAL-Link; Alma/SFX Local Collection |
| subjects | Absorption spectra Astronomy Carbon Earth, ocean, space Emission spectra Exact sciences and technology Hydrogen Line spectra R Coronae Borealis variables Spectral bands Stars Stellar spectra Stellar spectral lines Unusual and peculiar variables Variable and peculiar stars (including novae) |
| title | On the 1893 Absorption-Line Spectrum of Eta Carinae |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-09T17%3A50%3A34IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-jstor_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=On%20the%201893%20Absorption-Line%20Spectrum%20of%20Eta%20Carinae&rft.jtitle=Publications%20of%20the%20Astronomical%20Society%20of%20the%20Pacific&rft.au=Bidelman,%20William%20P.&rft.date=1993-06-01&rft.volume=105&rft.issue=688&rft.spage=578&rft.epage=578&rft.pages=578-578&rft.issn=0004-6280&rft.eissn=1538-3873&rft.coden=PASPAU&rft_id=info:doi/10.1086/133197&rft_dat=%3Cjstor_cross%3E40680073%3C/jstor_cross%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=40680073&rfr_iscdi=true |