THE OPEN CLUSTER NGC 3293 AND THE OB COMPLEX IN CARINA
Photoelectric measures in UBVRI of 46 stars in and around the open cluster NGC 3293 are presented. A distance modulus of Vo — Mv = 12.1 ± 0.15 (s.d.), corresponding to 2.6 kpc, was derived from the photometric data for 34 member stars. This is similar to distances found for other young groups in the...
Gespeichert in:
Veröffentlicht in: | Publications of the Astronomical Society of the Pacific 1980-06, Vol.92 (547), p.266-274 |
---|---|
Hauptverfasser: | , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 274 |
---|---|
container_issue | 547 |
container_start_page | 266 |
container_title | Publications of the Astronomical Society of the Pacific |
container_volume | 92 |
creator | FEINSTEIN, ALEJANDRO MARRACO, HUGO G. |
description | Photoelectric measures in UBVRI of 46 stars in and around the open cluster NGC 3293 are presented. A distance modulus of Vo — Mv = 12.1 ± 0.15 (s.d.), corresponding to 2.6 kpc, was derived from the photometric data for 34 member stars. This is similar to distances found for other young groups in the Carina region. One M supergiant and one Be star are members of the cluster. The brightest stars on the main sequence are of type B1. Several stars that have evolved away from the upper main sequence have been classified as giants and supergiants. The age of the cluster is about 7 x 10⁶ years. The star HD 91824 (no. 1), spectral type O7 V((f)), is not a member of the group. The interstellar reddening is normal in front of this cluster. |
doi_str_mv | 10.1086/130662 |
format | Article |
fullrecord | <record><control><sourceid>jstor_cross</sourceid><recordid>TN_cdi_crossref_primary_10_1086_130662</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><jstor_id>40677576</jstor_id><sourcerecordid>40677576</sourcerecordid><originalsourceid>FETCH-LOGICAL-c175t-2c92dff474d53cf62743b380483d2671c57181a4d3babe84fd567ff4393837433</originalsourceid><addsrcrecordid>eNo9z81Kw0AUBeBBKphWfQNhVu6id-bOX5ZxjG0gJqWm4C4kmQxYlEqmG9_eaMTVWZyPyz2EXDO4Y2DUPUNQip-RiEk0MRqNCxIBgIgVN3BBliEcABgzDCKi6k1Gq21WUlvsX-psR8u1pcgTpGn5SH_bB2qr522RvdJ8YukuL9NLcu7b9zBc_eWK7J-y2m7iolrnNi3inml5inmfcOe90MJJ7L3iWmCHBoRBx5VmvdTTG61w2LXdYIR3UunJY4IGJ4srcjvf7cdjCOPgm8_x7aMdvxoGzc_aZl47wZsZHsLpOP4rAUprqRV-A--FSA8</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>THE OPEN CLUSTER NGC 3293 AND THE OB COMPLEX IN CARINA</title><source>JSTOR Archive Collection A-Z Listing</source><source>Institute of Physics Journals</source><source>EZB-FREE-00999 freely available EZB journals</source><source>Alma/SFX Local Collection</source><creator>FEINSTEIN, ALEJANDRO ; MARRACO, HUGO G.</creator><creatorcontrib>FEINSTEIN, ALEJANDRO ; MARRACO, HUGO G.</creatorcontrib><description>Photoelectric measures in UBVRI of 46 stars in and around the open cluster NGC 3293 are presented. A distance modulus of Vo — Mv = 12.1 ± 0.15 (s.d.), corresponding to 2.6 kpc, was derived from the photometric data for 34 member stars. This is similar to distances found for other young groups in the Carina region. One M supergiant and one Be star are members of the cluster. The brightest stars on the main sequence are of type B1. Several stars that have evolved away from the upper main sequence have been classified as giants and supergiants. The age of the cluster is about 7 x 10⁶ years. The star HD 91824 (no. 1), spectral type O7 V((f)), is not a member of the group. The interstellar reddening is normal in front of this cluster.</description><identifier>ISSN: 0004-6280</identifier><identifier>EISSN: 1538-3873</identifier><identifier>DOI: 10.1086/130662</identifier><language>eng</language><publisher>The Astronomical Society of the Pacific</publisher><subject>Astronomical objects ; Interstellar reddening ; M supergiants ; Main sequence stars ; Open star clusters ; Radial velocity ; Stars ; Stellar classification ; Supergiant stars ; Variable stars</subject><ispartof>Publications of the Astronomical Society of the Pacific, 1980-06, Vol.92 (547), p.266-274</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c175t-2c92dff474d53cf62743b380483d2671c57181a4d3babe84fd567ff4393837433</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/40677576$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/40677576$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>314,780,784,803,27924,27925,58017,58250</link.rule.ids></links><search><creatorcontrib>FEINSTEIN, ALEJANDRO</creatorcontrib><creatorcontrib>MARRACO, HUGO G.</creatorcontrib><title>THE OPEN CLUSTER NGC 3293 AND THE OB COMPLEX IN CARINA</title><title>Publications of the Astronomical Society of the Pacific</title><description>Photoelectric measures in UBVRI of 46 stars in and around the open cluster NGC 3293 are presented. A distance modulus of Vo — Mv = 12.1 ± 0.15 (s.d.), corresponding to 2.6 kpc, was derived from the photometric data for 34 member stars. This is similar to distances found for other young groups in the Carina region. One M supergiant and one Be star are members of the cluster. The brightest stars on the main sequence are of type B1. Several stars that have evolved away from the upper main sequence have been classified as giants and supergiants. The age of the cluster is about 7 x 10⁶ years. The star HD 91824 (no. 1), spectral type O7 V((f)), is not a member of the group. The interstellar reddening is normal in front of this cluster.</description><subject>Astronomical objects</subject><subject>Interstellar reddening</subject><subject>M supergiants</subject><subject>Main sequence stars</subject><subject>Open star clusters</subject><subject>Radial velocity</subject><subject>Stars</subject><subject>Stellar classification</subject><subject>Supergiant stars</subject><subject>Variable stars</subject><issn>0004-6280</issn><issn>1538-3873</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1980</creationdate><recordtype>article</recordtype><recordid>eNo9z81Kw0AUBeBBKphWfQNhVu6id-bOX5ZxjG0gJqWm4C4kmQxYlEqmG9_eaMTVWZyPyz2EXDO4Y2DUPUNQip-RiEk0MRqNCxIBgIgVN3BBliEcABgzDCKi6k1Gq21WUlvsX-psR8u1pcgTpGn5SH_bB2qr522RvdJ8YukuL9NLcu7b9zBc_eWK7J-y2m7iolrnNi3inml5inmfcOe90MJJ7L3iWmCHBoRBx5VmvdTTG61w2LXdYIR3UunJY4IGJ4srcjvf7cdjCOPgm8_x7aMdvxoGzc_aZl47wZsZHsLpOP4rAUprqRV-A--FSA8</recordid><startdate>19800601</startdate><enddate>19800601</enddate><creator>FEINSTEIN, ALEJANDRO</creator><creator>MARRACO, HUGO G.</creator><general>The Astronomical Society of the Pacific</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>19800601</creationdate><title>THE OPEN CLUSTER NGC 3293 AND THE OB COMPLEX IN CARINA</title><author>FEINSTEIN, ALEJANDRO ; MARRACO, HUGO G.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c175t-2c92dff474d53cf62743b380483d2671c57181a4d3babe84fd567ff4393837433</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1980</creationdate><topic>Astronomical objects</topic><topic>Interstellar reddening</topic><topic>M supergiants</topic><topic>Main sequence stars</topic><topic>Open star clusters</topic><topic>Radial velocity</topic><topic>Stars</topic><topic>Stellar classification</topic><topic>Supergiant stars</topic><topic>Variable stars</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>FEINSTEIN, ALEJANDRO</creatorcontrib><creatorcontrib>MARRACO, HUGO G.</creatorcontrib><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>FEINSTEIN, ALEJANDRO</au><au>MARRACO, HUGO G.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>THE OPEN CLUSTER NGC 3293 AND THE OB COMPLEX IN CARINA</atitle><jtitle>Publications of the Astronomical Society of the Pacific</jtitle><date>1980-06-01</date><risdate>1980</risdate><volume>92</volume><issue>547</issue><spage>266</spage><epage>274</epage><pages>266-274</pages><issn>0004-6280</issn><eissn>1538-3873</eissn><abstract>Photoelectric measures in UBVRI of 46 stars in and around the open cluster NGC 3293 are presented. A distance modulus of Vo — Mv = 12.1 ± 0.15 (s.d.), corresponding to 2.6 kpc, was derived from the photometric data for 34 member stars. This is similar to distances found for other young groups in the Carina region. One M supergiant and one Be star are members of the cluster. The brightest stars on the main sequence are of type B1. Several stars that have evolved away from the upper main sequence have been classified as giants and supergiants. The age of the cluster is about 7 x 10⁶ years. The star HD 91824 (no. 1), spectral type O7 V((f)), is not a member of the group. The interstellar reddening is normal in front of this cluster.</abstract><pub>The Astronomical Society of the Pacific</pub><doi>10.1086/130662</doi><tpages>9</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0004-6280 |
ispartof | Publications of the Astronomical Society of the Pacific, 1980-06, Vol.92 (547), p.266-274 |
issn | 0004-6280 1538-3873 |
language | eng |
recordid | cdi_crossref_primary_10_1086_130662 |
source | JSTOR Archive Collection A-Z Listing; Institute of Physics Journals; EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection |
subjects | Astronomical objects Interstellar reddening M supergiants Main sequence stars Open star clusters Radial velocity Stars Stellar classification Supergiant stars Variable stars |
title | THE OPEN CLUSTER NGC 3293 AND THE OB COMPLEX IN CARINA |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-25T14%3A18%3A03IST&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=THE%20OPEN%20CLUSTER%20NGC%203293%20AND%20THE%20OB%20COMPLEX%20IN%20CARINA&rft.jtitle=Publications%20of%20the%20Astronomical%20Society%20of%20the%20Pacific&rft.au=FEINSTEIN,%20ALEJANDRO&rft.date=1980-06-01&rft.volume=92&rft.issue=547&rft.spage=266&rft.epage=274&rft.pages=266-274&rft.issn=0004-6280&rft.eissn=1538-3873&rft_id=info:doi/10.1086/130662&rft_dat=%3Cjstor_cross%3E40677576%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=40677576&rfr_iscdi=true |