Photometry of Praesepe in BVRI colors
Results are reported for BVRI photoelectric photometry of 55 stars in the region of the Praesepe cluster. Distance moduli are derived independently from V, B-V and V, R-I diagrams. These diagrams indicate that five of the stars do not appear to be cluster members and that 13 others are possibly bina...
Gespeichert in:
| Veröffentlicht in: | Astron. J.; (United States) 1979-10, Vol.84, p.1586-1590 |
|---|---|
| Hauptverfasser: | , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 1590 |
|---|---|
| container_issue | |
| container_start_page | 1586 |
| container_title | Astron. J.; (United States) |
| container_volume | 84 |
| creator | Upgren, A. R. Weis, E. W. Deluca, E. E. |
| description | Results are reported for BVRI photoelectric photometry of 55 stars in the region of the Praesepe cluster. Distance moduli are derived independently from V, B-V and V, R-I diagrams. These diagrams indicate that five of the stars do not appear to be cluster members and that 13 others are possibly binary members of Praesepe. The remaining stars are found to define a sequence similar in slope to that of the Hyades and lying 3.0 mag below it. Best values of 6.20 + or - 0.05 mag for the modulus and 174 + or - 4 pc for the distance of Praesepe are adopted. |
| doi_str_mv | 10.1086/112580 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_proquest_miscellaneous_23533016</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>23533016</sourcerecordid><originalsourceid>FETCH-LOGICAL-c243t-71525d2eda303cc70c34a0fb4adc1399137a59b9eb32e2b2e8ecc50f2b0fd6fb3</originalsourceid><addsrcrecordid>eNpF0E1LAzEUheEsFKxVf8Mg6G70JncyH0stfhQKFlG3IXPnho5MJ2OSLvrvVSq4OpuHs3iFuJBwI6Eub6VUuoYjMQOAIi-VLk_EaYyfAFLWUMzE1Xrjk99yCvvMu2wdLEeeOOvH7P7jdZmRH3yIZ-LY2SHy-d_Oxfvjw9viOV-9PC0Xd6ucVIEpr6RWulPcWQQkqoCwsODawnYksWkkVlY3bcMtKlat4pqJNDjVgutK1-JcXB5-fUy9idQnpg35cWRKRlcNYFn9oOsDmoL_2nFMZttH4mGwI_tdNAo1IsjyH1LwMQZ2Zgr91oa9kWB-85hDHvwGzGNWzA</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>23533016</pqid></control><display><type>article</type><title>Photometry of Praesepe in BVRI colors</title><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>Alma/SFX Local Collection</source><creator>Upgren, A. R. ; Weis, E. W. ; Deluca, E. E.</creator><creatorcontrib>Upgren, A. R. ; Weis, E. W. ; Deluca, E. E. ; Van Vleck Observatory, Wesleyan University, Middletown, Connecticut 06457</creatorcontrib><description>Results are reported for BVRI photoelectric photometry of 55 stars in the region of the Praesepe cluster. Distance moduli are derived independently from V, B-V and V, R-I diagrams. These diagrams indicate that five of the stars do not appear to be cluster members and that 13 others are possibly binary members of Praesepe. The remaining stars are found to define a sequence similar in slope to that of the Hyades and lying 3.0 mag below it. Best values of 6.20 + or - 0.05 mag for the modulus and 174 + or - 4 pc for the distance of Praesepe are adopted.</description><identifier>ISSN: 0004-6256</identifier><identifier>DOI: 10.1086/112580</identifier><language>eng</language><publisher>United States</publisher><subject>640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources ; BINARY STARS ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; MAIN SEQUENCE STARS ; MOTION ; PHOTOMETRY ; PROPER MOTION ; STAR CLUSTERS ; STARS</subject><ispartof>Astron. J.; (United States), 1979-10, Vol.84, p.1586-1590</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c243t-71525d2eda303cc70c34a0fb4adc1399137a59b9eb32e2b2e8ecc50f2b0fd6fb3</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/5790367$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Upgren, A. R.</creatorcontrib><creatorcontrib>Weis, E. W.</creatorcontrib><creatorcontrib>Deluca, E. E.</creatorcontrib><creatorcontrib>Van Vleck Observatory, Wesleyan University, Middletown, Connecticut 06457</creatorcontrib><title>Photometry of Praesepe in BVRI colors</title><title>Astron. J.; (United States)</title><description>Results are reported for BVRI photoelectric photometry of 55 stars in the region of the Praesepe cluster. Distance moduli are derived independently from V, B-V and V, R-I diagrams. These diagrams indicate that five of the stars do not appear to be cluster members and that 13 others are possibly binary members of Praesepe. The remaining stars are found to define a sequence similar in slope to that of the Hyades and lying 3.0 mag below it. Best values of 6.20 + or - 0.05 mag for the modulus and 174 + or - 4 pc for the distance of Praesepe are adopted.</description><subject>640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources</subject><subject>BINARY STARS</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>MAIN SEQUENCE STARS</subject><subject>MOTION</subject><subject>PHOTOMETRY</subject><subject>PROPER MOTION</subject><subject>STAR CLUSTERS</subject><subject>STARS</subject><issn>0004-6256</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1979</creationdate><recordtype>article</recordtype><recordid>eNpF0E1LAzEUheEsFKxVf8Mg6G70JncyH0stfhQKFlG3IXPnho5MJ2OSLvrvVSq4OpuHs3iFuJBwI6Eub6VUuoYjMQOAIi-VLk_EaYyfAFLWUMzE1Xrjk99yCvvMu2wdLEeeOOvH7P7jdZmRH3yIZ-LY2SHy-d_Oxfvjw9viOV-9PC0Xd6ucVIEpr6RWulPcWQQkqoCwsODawnYksWkkVlY3bcMtKlat4pqJNDjVgutK1-JcXB5-fUy9idQnpg35cWRKRlcNYFn9oOsDmoL_2nFMZttH4mGwI_tdNAo1IsjyH1LwMQZ2Zgr91oa9kWB-85hDHvwGzGNWzA</recordid><startdate>19791001</startdate><enddate>19791001</enddate><creator>Upgren, A. R.</creator><creator>Weis, E. W.</creator><creator>Deluca, E. E.</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>19791001</creationdate><title>Photometry of Praesepe in BVRI colors</title><author>Upgren, A. R. ; Weis, E. W. ; Deluca, E. E.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c243t-71525d2eda303cc70c34a0fb4adc1399137a59b9eb32e2b2e8ecc50f2b0fd6fb3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1979</creationdate><topic>640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources</topic><topic>BINARY STARS</topic><topic>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</topic><topic>MAIN SEQUENCE STARS</topic><topic>MOTION</topic><topic>PHOTOMETRY</topic><topic>PROPER MOTION</topic><topic>STAR CLUSTERS</topic><topic>STARS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Upgren, A. R.</creatorcontrib><creatorcontrib>Weis, E. W.</creatorcontrib><creatorcontrib>Deluca, E. E.</creatorcontrib><creatorcontrib>Van Vleck Observatory, Wesleyan University, Middletown, Connecticut 06457</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>Astron. J.; (United States)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Upgren, A. R.</au><au>Weis, E. W.</au><au>Deluca, E. E.</au><aucorp>Van Vleck Observatory, Wesleyan University, Middletown, Connecticut 06457</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Photometry of Praesepe in BVRI colors</atitle><jtitle>Astron. J.; (United States)</jtitle><date>1979-10-01</date><risdate>1979</risdate><volume>84</volume><spage>1586</spage><epage>1590</epage><pages>1586-1590</pages><issn>0004-6256</issn><abstract>Results are reported for BVRI photoelectric photometry of 55 stars in the region of the Praesepe cluster. Distance moduli are derived independently from V, B-V and V, R-I diagrams. These diagrams indicate that five of the stars do not appear to be cluster members and that 13 others are possibly binary members of Praesepe. The remaining stars are found to define a sequence similar in slope to that of the Hyades and lying 3.0 mag below it. Best values of 6.20 + or - 0.05 mag for the modulus and 174 + or - 4 pc for the distance of Praesepe are adopted.</abstract><cop>United States</cop><doi>10.1086/112580</doi><tpages>5</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0004-6256 |
| ispartof | Astron. J.; (United States), 1979-10, Vol.84, p.1586-1590 |
| issn | 0004-6256 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_23533016 |
| source | Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Alma/SFX Local Collection |
| subjects | 640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources BINARY STARS CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS MAIN SEQUENCE STARS MOTION PHOTOMETRY PROPER MOTION STAR CLUSTERS STARS |
| title | Photometry of Praesepe in BVRI colors |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-04T03%3A06%3A55IST&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=Photometry%20of%20Praesepe%20in%20BVRI%20colors&rft.jtitle=Astron.%20J.;%20(United%20States)&rft.au=Upgren,%20A.%20R.&rft.aucorp=Van%20Vleck%20Observatory,%20Wesleyan%20University,%20Middletown,%20Connecticut%2006457&rft.date=1979-10-01&rft.volume=84&rft.spage=1586&rft.epage=1590&rft.pages=1586-1590&rft.issn=0004-6256&rft_id=info:doi/10.1086/112580&rft_dat=%3Cproquest_osti_%3E23533016%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=23533016&rft_id=info:pmid/&rfr_iscdi=true |