The short-period Cepheid EU Tau. II - Physical properties of the star
A surface brightness analysis on the photometric and radial-velocity data of EU Tau presented by Gieren et al. (1989) is presented. The stellar radius and distance are determined with a 5 percent precision. The radius and distance results are used to establish the fundamental stellar parameters, inc...
Gespeichert in:
Veröffentlicht in: | The Astronomical journal 1990-04, Vol.99, p.1196-1206 |
---|---|
Hauptverfasser: | , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 1206 |
---|---|
container_issue | |
container_start_page | 1196 |
container_title | The Astronomical journal |
container_volume | 99 |
creator | Gieren, Wolfgang P. Moffett, Thomas J. Barnes, Thomas G., III Frueh, Marian L. Matthews, Jaymie M. |
description | A surface brightness analysis on the photometric and radial-velocity data of EU Tau presented by Gieren et al. (1989) is presented. The stellar radius and distance are determined with a 5 percent precision. The radius and distance results are used to establish the fundamental stellar parameters, including luminosity, mass, effective temperature, and binary status. The results strongly suggest that EU Tau is pulsating in the radial first overtone mode. (R.B.) |
doi_str_mv | 10.1086/115408 |
format | Article |
fullrecord | <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_7041762</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>25049942</sourcerecordid><originalsourceid>FETCH-LOGICAL-c194t-4c18d23e7a115209fb1d765530f1b1e47cd7fd4e029815d0d6f29b9b4580e3f63</originalsourceid><addsrcrecordid>eNpNkLFOwzAURS0EEqXAN1gMbCnvJXbijKgqUKkSDO1sJfaLYpTWwXaH_j2pysB0l3Ovji5jjwgLBFW-IEoB6orNUBYqK5TCazYDAJGVuSxv2V2M3wCICsSMrbY98dj7kLKRgvOWL2nsyVm-2vFtc1zw9Zpn_Ks_RWeagY_BT1xyFLnveDqXUxPu2U3XDJEe_nLOdm-r7fIj23y-r5evm8xgLVImDCqbF1Q1k2MOddeirUopC-iwRRKVsVVnBUFeK5QWbNnldVu3QiqgoiuLOXu67PqYnI7GJTK98YcDmaQrEFiV-QQ9X6DJ9edIMem9i4aGoTmQP0adSxB1Lf6BJvgYA3V6DG7fhJNG0Ocr9eXK4hc73WI-</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>25049942</pqid></control><display><type>article</type><title>The short-period Cepheid EU Tau. II - Physical properties of the star</title><source>EZB-FREE-00999 freely available EZB journals</source><source>Alma/SFX Local Collection</source><creator>Gieren, Wolfgang P. ; Moffett, Thomas J. ; Barnes, Thomas G., III ; Frueh, Marian L. ; Matthews, Jaymie M.</creator><creatorcontrib>Gieren, Wolfgang P. ; Moffett, Thomas J. ; Barnes, Thomas G., III ; Frueh, Marian L. ; Matthews, Jaymie M.</creatorcontrib><description>A surface brightness analysis on the photometric and radial-velocity data of EU Tau presented by Gieren et al. (1989) is presented. The stellar radius and distance are determined with a 5 percent precision. The radius and distance results are used to establish the fundamental stellar parameters, including luminosity, mass, effective temperature, and binary status. The results strongly suggest that EU Tau is pulsating in the radial first overtone mode. (R.B.)</description><identifier>ISSN: 0004-6256</identifier><identifier>EISSN: 1538-3881</identifier><identifier>DOI: 10.1086/115408</identifier><language>eng</language><publisher>United States</publisher><subject>640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources ; BINARY STARS ; BRIGHTNESS ; CEPHEIDS ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; DIAGRAMS ; DISTANCE ; HERTZSPRUNG-RUSSELL DIAGRAM ; LUMINOSITY ; MASS ; OPTICAL PROPERTIES ; PHYSICAL PROPERTIES ; PULSATING VARIABLE STARS ; RADIAL VELOCITY ; SIZE ; SPECTROPHOTOMETRY ; STARS ; VARIABLE STARS ; VELOCITY</subject><ispartof>The Astronomical journal, 1990-04, Vol.99, p.1196-1206</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c194t-4c18d23e7a115209fb1d765530f1b1e47cd7fd4e029815d0d6f29b9b4580e3f63</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,27903,27904</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/7041762$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Gieren, Wolfgang P.</creatorcontrib><creatorcontrib>Moffett, Thomas J.</creatorcontrib><creatorcontrib>Barnes, Thomas G., III</creatorcontrib><creatorcontrib>Frueh, Marian L.</creatorcontrib><creatorcontrib>Matthews, Jaymie M.</creatorcontrib><title>The short-period Cepheid EU Tau. II - Physical properties of the star</title><title>The Astronomical journal</title><description>A surface brightness analysis on the photometric and radial-velocity data of EU Tau presented by Gieren et al. (1989) is presented. The stellar radius and distance are determined with a 5 percent precision. The radius and distance results are used to establish the fundamental stellar parameters, including luminosity, mass, effective temperature, and binary status. The results strongly suggest that EU Tau is pulsating in the radial first overtone mode. (R.B.)</description><subject>640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources</subject><subject>BINARY STARS</subject><subject>BRIGHTNESS</subject><subject>CEPHEIDS</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>DIAGRAMS</subject><subject>DISTANCE</subject><subject>HERTZSPRUNG-RUSSELL DIAGRAM</subject><subject>LUMINOSITY</subject><subject>MASS</subject><subject>OPTICAL PROPERTIES</subject><subject>PHYSICAL PROPERTIES</subject><subject>PULSATING VARIABLE STARS</subject><subject>RADIAL VELOCITY</subject><subject>SIZE</subject><subject>SPECTROPHOTOMETRY</subject><subject>STARS</subject><subject>VARIABLE STARS</subject><subject>VELOCITY</subject><issn>0004-6256</issn><issn>1538-3881</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1990</creationdate><recordtype>article</recordtype><recordid>eNpNkLFOwzAURS0EEqXAN1gMbCnvJXbijKgqUKkSDO1sJfaLYpTWwXaH_j2pysB0l3Ovji5jjwgLBFW-IEoB6orNUBYqK5TCazYDAJGVuSxv2V2M3wCICsSMrbY98dj7kLKRgvOWL2nsyVm-2vFtc1zw9Zpn_Ks_RWeagY_BT1xyFLnveDqXUxPu2U3XDJEe_nLOdm-r7fIj23y-r5evm8xgLVImDCqbF1Q1k2MOddeirUopC-iwRRKVsVVnBUFeK5QWbNnldVu3QiqgoiuLOXu67PqYnI7GJTK98YcDmaQrEFiV-QQ9X6DJ9edIMem9i4aGoTmQP0adSxB1Lf6BJvgYA3V6DG7fhJNG0Ocr9eXK4hc73WI-</recordid><startdate>19900401</startdate><enddate>19900401</enddate><creator>Gieren, Wolfgang P.</creator><creator>Moffett, Thomas J.</creator><creator>Barnes, Thomas G., III</creator><creator>Frueh, Marian L.</creator><creator>Matthews, Jaymie M.</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>19900401</creationdate><title>The short-period Cepheid EU Tau. II - Physical properties of the star</title><author>Gieren, Wolfgang P. ; Moffett, Thomas J. ; Barnes, Thomas G., III ; Frueh, Marian L. ; Matthews, Jaymie M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c194t-4c18d23e7a115209fb1d765530f1b1e47cd7fd4e029815d0d6f29b9b4580e3f63</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1990</creationdate><topic>640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources</topic><topic>BINARY STARS</topic><topic>BRIGHTNESS</topic><topic>CEPHEIDS</topic><topic>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</topic><topic>DIAGRAMS</topic><topic>DISTANCE</topic><topic>HERTZSPRUNG-RUSSELL DIAGRAM</topic><topic>LUMINOSITY</topic><topic>MASS</topic><topic>OPTICAL PROPERTIES</topic><topic>PHYSICAL PROPERTIES</topic><topic>PULSATING VARIABLE STARS</topic><topic>RADIAL VELOCITY</topic><topic>SIZE</topic><topic>SPECTROPHOTOMETRY</topic><topic>STARS</topic><topic>VARIABLE STARS</topic><topic>VELOCITY</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gieren, Wolfgang P.</creatorcontrib><creatorcontrib>Moffett, Thomas J.</creatorcontrib><creatorcontrib>Barnes, Thomas G., III</creatorcontrib><creatorcontrib>Frueh, Marian L.</creatorcontrib><creatorcontrib>Matthews, Jaymie M.</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>The Astronomical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gieren, Wolfgang P.</au><au>Moffett, Thomas J.</au><au>Barnes, Thomas G., III</au><au>Frueh, Marian L.</au><au>Matthews, Jaymie M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The short-period Cepheid EU Tau. II - Physical properties of the star</atitle><jtitle>The Astronomical journal</jtitle><date>1990-04-01</date><risdate>1990</risdate><volume>99</volume><spage>1196</spage><epage>1206</epage><pages>1196-1206</pages><issn>0004-6256</issn><eissn>1538-3881</eissn><abstract>A surface brightness analysis on the photometric and radial-velocity data of EU Tau presented by Gieren et al. (1989) is presented. The stellar radius and distance are determined with a 5 percent precision. The radius and distance results are used to establish the fundamental stellar parameters, including luminosity, mass, effective temperature, and binary status. The results strongly suggest that EU Tau is pulsating in the radial first overtone mode. (R.B.)</abstract><cop>United States</cop><doi>10.1086/115408</doi><tpages>11</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0004-6256 |
ispartof | The Astronomical journal, 1990-04, Vol.99, p.1196-1206 |
issn | 0004-6256 1538-3881 |
language | eng |
recordid | cdi_osti_scitechconnect_7041762 |
source | EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection |
subjects | 640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources BINARY STARS BRIGHTNESS CEPHEIDS CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS DIAGRAMS DISTANCE HERTZSPRUNG-RUSSELL DIAGRAM LUMINOSITY MASS OPTICAL PROPERTIES PHYSICAL PROPERTIES PULSATING VARIABLE STARS RADIAL VELOCITY SIZE SPECTROPHOTOMETRY STARS VARIABLE STARS VELOCITY |
title | The short-period Cepheid EU Tau. II - Physical properties of the star |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-26T16%3A03%3A13IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20short-period%20Cepheid%20EU%20Tau.%20II%20-%20Physical%20properties%20of%20the%20star&rft.jtitle=The%20Astronomical%20journal&rft.au=Gieren,%20Wolfgang%20P.&rft.date=1990-04-01&rft.volume=99&rft.spage=1196&rft.epage=1206&rft.pages=1196-1206&rft.issn=0004-6256&rft.eissn=1538-3881&rft_id=info:doi/10.1086/115408&rft_dat=%3Cproquest_osti_%3E25049942%3C/proquest_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=25049942&rft_id=info:pmid/&rfr_iscdi=true |