Studies of nearby poor clusters - A3574 and S753
Photometric and spectroscopic data are presented for two clusters, A3574 and S753, belonging to the Centaurus concentration of galaxies. The masses of the clusters are estimated at 1.5 x 10 to the 14th solar masses; no evidence of substructure has been detected in either cluster. The solution of a t...
Gespeichert in:
| Veröffentlicht in: | The Astronomical journal 1991-01, Vol.101, p.57-65 |
|---|---|
| Hauptverfasser: | , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 65 |
|---|---|
| container_issue | |
| container_start_page | 57 |
| container_title | The Astronomical journal |
| container_volume | 101 |
| creator | Willmer, C. N. A. Focardi, P. Chan, R. Pellegrini, P. S. da Costa, Nicolaci L. |
| description | Photometric and spectroscopic data are presented for two clusters, A3574 and S753, belonging to the Centaurus concentration of galaxies. The masses of the clusters are estimated at 1.5 x 10 to the 14th solar masses; no evidence of substructure has been detected in either cluster. The solution of a two-body linear orbit suggests that the clusters do not form a bound system, although the result is marginal. (V.L.) |
| doi_str_mv | 10.1086/115665 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_6159113</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>25448916</sourcerecordid><originalsourceid>FETCH-LOGICAL-c311t-cebec4c51b6d7c7ed8896b946cd1577098b232838b4899c0fee2144293dc85083</originalsourceid><addsrcrecordid>eNpFkD1PwzAUAC0EEqXAb7AY2AJ-8UfssaqgIFViKMxW8vIigtI42M7Qf09RkZhuOd1wjN2CeABhzSOANkafsQVoaQtpLZyzhRBCFabU5pJdpfQlBIAVasHELs9tT4mHjo9Ux-bApxAix2FOmWLiBV9JXSlejy3fVVpes4uuHhLd_HHJPp6f3tcvxfZt87pebQuUALlAaggVamhMW2FFrbXONE4ZbEFXlXC2KWVppW2UdQ5FR1SCUqWTLVotrFyyu1M3pNz7hH0m_MQwjoTZG9AOQB6l-5M0xfA9U8p-3yekYahHCnPypVbHPJh_EWNIKVLnp9jv63jwIPzvNX-6Jn8AvYdaBg</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>25448916</pqid></control><display><type>article</type><title>Studies of nearby poor clusters - A3574 and S753</title><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>Alma/SFX Local Collection</source><creator>Willmer, C. N. A. ; Focardi, P. ; Chan, R. ; Pellegrini, P. S. ; da Costa, Nicolaci L.</creator><creatorcontrib>Willmer, C. N. A. ; Focardi, P. ; Chan, R. ; Pellegrini, P. S. ; da Costa, Nicolaci L.</creatorcontrib><description>Photometric and spectroscopic data are presented for two clusters, A3574 and S753, belonging to the Centaurus concentration of galaxies. The masses of the clusters are estimated at 1.5 x 10 to the 14th solar masses; no evidence of substructure has been detected in either cluster. The solution of a two-body linear orbit suggests that the clusters do not form a bound system, although the result is marginal. (V.L.)</description><identifier>ISSN: 0004-6256</identifier><identifier>EISSN: 1538-3881</identifier><identifier>DOI: 10.1086/115665</identifier><language>eng</language><publisher>United States</publisher><subject>640105 - Astrophysics & Cosmology- Galaxies ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; GALAXY CLUSTERS ; LUMINOSITY ; MANY-BODY PROBLEM ; MASS ; MORPHOLOGY ; MOTION ; OPTICAL PROPERTIES ; PHOTOGRAPHY ; PHOTOMETRY ; PHYSICAL PROPERTIES ; ROTATION ; SPECTROSCOPY ; TWO-BODY PROBLEM</subject><ispartof>The Astronomical journal, 1991-01, Vol.101, p.57-65</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c311t-cebec4c51b6d7c7ed8896b946cd1577098b232838b4899c0fee2144293dc85083</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,315,782,786,887,27931,27932</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/6159113$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Willmer, C. N. A.</creatorcontrib><creatorcontrib>Focardi, P.</creatorcontrib><creatorcontrib>Chan, R.</creatorcontrib><creatorcontrib>Pellegrini, P. S.</creatorcontrib><creatorcontrib>da Costa, Nicolaci L.</creatorcontrib><title>Studies of nearby poor clusters - A3574 and S753</title><title>The Astronomical journal</title><description>Photometric and spectroscopic data are presented for two clusters, A3574 and S753, belonging to the Centaurus concentration of galaxies. The masses of the clusters are estimated at 1.5 x 10 to the 14th solar masses; no evidence of substructure has been detected in either cluster. The solution of a two-body linear orbit suggests that the clusters do not form a bound system, although the result is marginal. (V.L.)</description><subject>640105 - Astrophysics & Cosmology- Galaxies</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>GALAXY CLUSTERS</subject><subject>LUMINOSITY</subject><subject>MANY-BODY PROBLEM</subject><subject>MASS</subject><subject>MORPHOLOGY</subject><subject>MOTION</subject><subject>OPTICAL PROPERTIES</subject><subject>PHOTOGRAPHY</subject><subject>PHOTOMETRY</subject><subject>PHYSICAL PROPERTIES</subject><subject>ROTATION</subject><subject>SPECTROSCOPY</subject><subject>TWO-BODY PROBLEM</subject><issn>0004-6256</issn><issn>1538-3881</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1991</creationdate><recordtype>article</recordtype><recordid>eNpFkD1PwzAUAC0EEqXAb7AY2AJ-8UfssaqgIFViKMxW8vIigtI42M7Qf09RkZhuOd1wjN2CeABhzSOANkafsQVoaQtpLZyzhRBCFabU5pJdpfQlBIAVasHELs9tT4mHjo9Ux-bApxAix2FOmWLiBV9JXSlejy3fVVpes4uuHhLd_HHJPp6f3tcvxfZt87pebQuUALlAaggVamhMW2FFrbXONE4ZbEFXlXC2KWVppW2UdQ5FR1SCUqWTLVotrFyyu1M3pNz7hH0m_MQwjoTZG9AOQB6l-5M0xfA9U8p-3yekYahHCnPypVbHPJh_EWNIKVLnp9jv63jwIPzvNX-6Jn8AvYdaBg</recordid><startdate>199101</startdate><enddate>199101</enddate><creator>Willmer, C. N. A.</creator><creator>Focardi, P.</creator><creator>Chan, R.</creator><creator>Pellegrini, P. S.</creator><creator>da Costa, Nicolaci L.</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>199101</creationdate><title>Studies of nearby poor clusters - A3574 and S753</title><author>Willmer, C. N. A. ; Focardi, P. ; Chan, R. ; Pellegrini, P. S. ; da Costa, Nicolaci L.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c311t-cebec4c51b6d7c7ed8896b946cd1577098b232838b4899c0fee2144293dc85083</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1991</creationdate><topic>640105 - Astrophysics & Cosmology- Galaxies</topic><topic>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</topic><topic>GALAXY CLUSTERS</topic><topic>LUMINOSITY</topic><topic>MANY-BODY PROBLEM</topic><topic>MASS</topic><topic>MORPHOLOGY</topic><topic>MOTION</topic><topic>OPTICAL PROPERTIES</topic><topic>PHOTOGRAPHY</topic><topic>PHOTOMETRY</topic><topic>PHYSICAL PROPERTIES</topic><topic>ROTATION</topic><topic>SPECTROSCOPY</topic><topic>TWO-BODY PROBLEM</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Willmer, C. N. A.</creatorcontrib><creatorcontrib>Focardi, P.</creatorcontrib><creatorcontrib>Chan, R.</creatorcontrib><creatorcontrib>Pellegrini, P. S.</creatorcontrib><creatorcontrib>da Costa, Nicolaci L.</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>Willmer, C. N. A.</au><au>Focardi, P.</au><au>Chan, R.</au><au>Pellegrini, P. S.</au><au>da Costa, Nicolaci L.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Studies of nearby poor clusters - A3574 and S753</atitle><jtitle>The Astronomical journal</jtitle><date>1991-01</date><risdate>1991</risdate><volume>101</volume><spage>57</spage><epage>65</epage><pages>57-65</pages><issn>0004-6256</issn><eissn>1538-3881</eissn><abstract>Photometric and spectroscopic data are presented for two clusters, A3574 and S753, belonging to the Centaurus concentration of galaxies. The masses of the clusters are estimated at 1.5 x 10 to the 14th solar masses; no evidence of substructure has been detected in either cluster. The solution of a two-body linear orbit suggests that the clusters do not form a bound system, although the result is marginal. (V.L.)</abstract><cop>United States</cop><doi>10.1086/115665</doi><tpages>9</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0004-6256 |
| ispartof | The Astronomical journal, 1991-01, Vol.101, p.57-65 |
| issn | 0004-6256 1538-3881 |
| language | eng |
| recordid | cdi_osti_scitechconnect_6159113 |
| source | Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Alma/SFX Local Collection |
| subjects | 640105 - Astrophysics & Cosmology- Galaxies CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS GALAXY CLUSTERS LUMINOSITY MANY-BODY PROBLEM MASS MORPHOLOGY MOTION OPTICAL PROPERTIES PHOTOGRAPHY PHOTOMETRY PHYSICAL PROPERTIES ROTATION SPECTROSCOPY TWO-BODY PROBLEM |
| title | Studies of nearby poor clusters - A3574 and S753 |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-04T08%3A26%3A29IST&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=Studies%20of%20nearby%20poor%20clusters%20-%20A3574%20and%20S753&rft.jtitle=The%20Astronomical%20journal&rft.au=Willmer,%20C.%20N.%20A.&rft.date=1991-01&rft.volume=101&rft.spage=57&rft.epage=65&rft.pages=57-65&rft.issn=0004-6256&rft.eissn=1538-3881&rft_id=info:doi/10.1086/115665&rft_dat=%3Cproquest_osti_%3E25448916%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=25448916&rft_id=info:pmid/&rfr_iscdi=true |