The angular momentum of eclipsing binaries
An observational diagram for eclipsing binary systems is presented in order to provide fundamental data for a relationship between the angular momenta (J) and the mass (M). J is quantified for a circular orbit and relations are defined among the orbital radii relative to the gravity center, the comp...
Gespeichert in:
Veröffentlicht in: | Astrophysics and space science 1983-07, Vol.94 (1), p.165-170 |
---|---|
Hauptverfasser: | , |
Format: | Artikel |
Sprache: | eng |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 170 |
---|---|
container_issue | 1 |
container_start_page | 165 |
container_title | Astrophysics and space science |
container_volume | 94 |
creator | Sister, R. F. Marton, S. |
description | An observational diagram for eclipsing binary systems is presented in order to provide fundamental data for a relationship between the angular momenta (J) and the mass (M). J is quantified for a circular orbit and relations are defined among the orbital radii relative to the gravity center, the components' masses, the total mass, and the mass ratio. An equation is described and used to obtain the J value for 1048 eclipsing binaries, and J-M diagrams are generated for detached, semi-detached, and contact systems. A slope for the three systems clusters around 1.92. Further applications of the diagrams to the local supercluster and the metagalaxy demonstrate that a universal cosmogonic mechanism may exist, which was predicted by the cosmological principle of a hadronic fireball. |
doi_str_mv | 10.1007/BF00651768 |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_24083592</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>24083592</sourcerecordid><originalsourceid>FETCH-LOGICAL-c262t-7fb9bdee410c74a10ce15fa97a6a9ca35a76eadfd3696fde24c49e39ff3986e63</originalsourceid><addsrcrecordid>eNpFkM1KAzEYRYMoWKsbn2BWLgqj-ZtkstRiVSi4qdBd-CbzpUbmz2Rm4ds7pYKbe7lwuItDyC2j94xS_fC0oVQVTKvyjCxYoXlupNqfkwWlVOZK0v0luUrpa55GGb0gq90nZtAdpgZi1vYtduPUZr3P0DVhSKE7ZFXoIAZM1-TCQ5Pw5q-X5GPzvFu_5tv3l7f14zZ3XPEx174yVY0oGXVawpzICg9GgwLjQBSgFULta6GM8jVy6aRBYbwXplSoxJLcnX6H2H9PmEbbhuSwaaDDfkqWS1qKwvAZXJ1AF_uUIno7xNBC_LGM2qMO-69D_AJOBFIn</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>24083592</pqid></control><display><type>article</type><title>The angular momentum of eclipsing binaries</title><source>SpringerLink Journals</source><source>EZB-FREE-00999 freely available EZB journals</source><creator>Sister, R. F. ; Marton, S.</creator><creatorcontrib>Sister, R. F. ; Marton, S.</creatorcontrib><description>An observational diagram for eclipsing binary systems is presented in order to provide fundamental data for a relationship between the angular momenta (J) and the mass (M). J is quantified for a circular orbit and relations are defined among the orbital radii relative to the gravity center, the components' masses, the total mass, and the mass ratio. An equation is described and used to obtain the J value for 1048 eclipsing binaries, and J-M diagrams are generated for detached, semi-detached, and contact systems. A slope for the three systems clusters around 1.92. Further applications of the diagrams to the local supercluster and the metagalaxy demonstrate that a universal cosmogonic mechanism may exist, which was predicted by the cosmological principle of a hadronic fireball.</description><identifier>ISSN: 0004-640X</identifier><identifier>EISSN: 1572-946X</identifier><identifier>DOI: 10.1007/BF00651768</identifier><language>eng</language><ispartof>Astrophysics and space science, 1983-07, Vol.94 (1), p.165-170</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c262t-7fb9bdee410c74a10ce15fa97a6a9ca35a76eadfd3696fde24c49e39ff3986e63</citedby><cites>FETCH-LOGICAL-c262t-7fb9bdee410c74a10ce15fa97a6a9ca35a76eadfd3696fde24c49e39ff3986e63</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Sister, R. F.</creatorcontrib><creatorcontrib>Marton, S.</creatorcontrib><title>The angular momentum of eclipsing binaries</title><title>Astrophysics and space science</title><description>An observational diagram for eclipsing binary systems is presented in order to provide fundamental data for a relationship between the angular momenta (J) and the mass (M). J is quantified for a circular orbit and relations are defined among the orbital radii relative to the gravity center, the components' masses, the total mass, and the mass ratio. An equation is described and used to obtain the J value for 1048 eclipsing binaries, and J-M diagrams are generated for detached, semi-detached, and contact systems. A slope for the three systems clusters around 1.92. Further applications of the diagrams to the local supercluster and the metagalaxy demonstrate that a universal cosmogonic mechanism may exist, which was predicted by the cosmological principle of a hadronic fireball.</description><issn>0004-640X</issn><issn>1572-946X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1983</creationdate><recordtype>article</recordtype><recordid>eNpFkM1KAzEYRYMoWKsbn2BWLgqj-ZtkstRiVSi4qdBd-CbzpUbmz2Rm4ds7pYKbe7lwuItDyC2j94xS_fC0oVQVTKvyjCxYoXlupNqfkwWlVOZK0v0luUrpa55GGb0gq90nZtAdpgZi1vYtduPUZr3P0DVhSKE7ZFXoIAZM1-TCQ5Pw5q-X5GPzvFu_5tv3l7f14zZ3XPEx174yVY0oGXVawpzICg9GgwLjQBSgFULta6GM8jVy6aRBYbwXplSoxJLcnX6H2H9PmEbbhuSwaaDDfkqWS1qKwvAZXJ1AF_uUIno7xNBC_LGM2qMO-69D_AJOBFIn</recordid><startdate>198307</startdate><enddate>198307</enddate><creator>Sister, R. F.</creator><creator>Marton, S.</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>198307</creationdate><title>The angular momentum of eclipsing binaries</title><author>Sister, R. F. ; Marton, S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c262t-7fb9bdee410c74a10ce15fa97a6a9ca35a76eadfd3696fde24c49e39ff3986e63</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1983</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Sister, R. F.</creatorcontrib><creatorcontrib>Marton, S.</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Astrophysics and space science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Sister, R. F.</au><au>Marton, S.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The angular momentum of eclipsing binaries</atitle><jtitle>Astrophysics and space science</jtitle><date>1983-07</date><risdate>1983</risdate><volume>94</volume><issue>1</issue><spage>165</spage><epage>170</epage><pages>165-170</pages><issn>0004-640X</issn><eissn>1572-946X</eissn><abstract>An observational diagram for eclipsing binary systems is presented in order to provide fundamental data for a relationship between the angular momenta (J) and the mass (M). J is quantified for a circular orbit and relations are defined among the orbital radii relative to the gravity center, the components' masses, the total mass, and the mass ratio. An equation is described and used to obtain the J value for 1048 eclipsing binaries, and J-M diagrams are generated for detached, semi-detached, and contact systems. A slope for the three systems clusters around 1.92. Further applications of the diagrams to the local supercluster and the metagalaxy demonstrate that a universal cosmogonic mechanism may exist, which was predicted by the cosmological principle of a hadronic fireball.</abstract><doi>10.1007/BF00651768</doi><tpages>6</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0004-640X |
ispartof | Astrophysics and space science, 1983-07, Vol.94 (1), p.165-170 |
issn | 0004-640X 1572-946X |
language | eng |
recordid | cdi_proquest_miscellaneous_24083592 |
source | SpringerLink Journals; EZB-FREE-00999 freely available EZB journals |
title | The angular momentum of eclipsing binaries |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-25T15%3A07%3A28IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20angular%20momentum%20of%20eclipsing%20binaries&rft.jtitle=Astrophysics%20and%20space%20science&rft.au=Sister,%20R.%20F.&rft.date=1983-07&rft.volume=94&rft.issue=1&rft.spage=165&rft.epage=170&rft.pages=165-170&rft.issn=0004-640X&rft.eissn=1572-946X&rft_id=info:doi/10.1007/BF00651768&rft_dat=%3Cproquest_cross%3E24083592%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=24083592&rft_id=info:pmid/&rfr_iscdi=true |