Loading…
Astrometric Measurement of the Double-Star System WDS 09168-3407 B 1118
We present updated measurements for the position angle and separation of the double-star WDS 09168-3407 B 1118, incorporating data from our observation, Gaia Early Data Release 3 mission, and historical records. Our findings indicate a position angle of 341.4{\deg} and separation of 3.36". Addi...
Saved in:
Published in: | arXiv.org 2024-03 |
---|---|
Main Authors: | , |
Format: | Article |
Language: | English |
Subjects: | |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | |
---|---|
cites | |
container_end_page | |
container_issue | |
container_start_page | |
container_title | arXiv.org |
container_volume | |
creator | Ibharalu, Elijah Miracle Chibuzor Marcel |
description | We present updated measurements for the position angle and separation of the double-star WDS 09168-3407 B 1118, incorporating data from our observation, Gaia Early Data Release 3 mission, and historical records. Our findings indicate a position angle of 341.4{\deg} and separation of 3.36". Additionally, we utilized parallax and the ratio of proper motion metric (rPM) values to evaluate the potential binarity of the system. Our analysis suggests that the system may be gravitationally bound. |
format | article |
fullrecord | <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2937449929</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2937449929</sourcerecordid><originalsourceid>FETCH-proquest_journals_29374499293</originalsourceid><addsrcrecordid>eNqNyrsKwjAUgOEgCBbtOxxwDuTWNhnVelmcKjiWKqdoaRvNZfDt7eADOH3D_89IIqTkVCshFiT1vmOMibwQWSYTctz44OyAwT3vcMbGR4cDjgFsC-GBUNp465FWoXFQfXzAAa5lBczwXFOpWAFb4JzrFZm3Te8x_bkk68P-sjvRl7PviD7UnY1unFItjCyUMmbyv-sLnZs4Lg</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2937449929</pqid></control><display><type>article</type><title>Astrometric Measurement of the Double-Star System WDS 09168-3407 B 1118</title><source>Publicly Available Content Database (Proquest) (PQ_SDU_P3)</source><creator>Ibharalu, Elijah ; Miracle Chibuzor Marcel</creator><creatorcontrib>Ibharalu, Elijah ; Miracle Chibuzor Marcel</creatorcontrib><description>We present updated measurements for the position angle and separation of the double-star WDS 09168-3407 B 1118, incorporating data from our observation, Gaia Early Data Release 3 mission, and historical records. Our findings indicate a position angle of 341.4{\deg} and separation of 3.36". Additionally, we utilized parallax and the ratio of proper motion metric (rPM) values to evaluate the potential binarity of the system. Our analysis suggests that the system may be gravitationally bound.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Parallax ; Position measurement ; Separation</subject><ispartof>arXiv.org, 2024-03</ispartof><rights>2024. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2937449929?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>780,784,25753,37012,44590</link.rule.ids></links><search><creatorcontrib>Ibharalu, Elijah</creatorcontrib><creatorcontrib>Miracle Chibuzor Marcel</creatorcontrib><title>Astrometric Measurement of the Double-Star System WDS 09168-3407 B 1118</title><title>arXiv.org</title><description>We present updated measurements for the position angle and separation of the double-star WDS 09168-3407 B 1118, incorporating data from our observation, Gaia Early Data Release 3 mission, and historical records. Our findings indicate a position angle of 341.4{\deg} and separation of 3.36". Additionally, we utilized parallax and the ratio of proper motion metric (rPM) values to evaluate the potential binarity of the system. Our analysis suggests that the system may be gravitationally bound.</description><subject>Parallax</subject><subject>Position measurement</subject><subject>Separation</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNqNyrsKwjAUgOEgCBbtOxxwDuTWNhnVelmcKjiWKqdoaRvNZfDt7eADOH3D_89IIqTkVCshFiT1vmOMibwQWSYTctz44OyAwT3vcMbGR4cDjgFsC-GBUNp465FWoXFQfXzAAa5lBczwXFOpWAFb4JzrFZm3Te8x_bkk68P-sjvRl7PviD7UnY1unFItjCyUMmbyv-sLnZs4Lg</recordid><startdate>20240301</startdate><enddate>20240301</enddate><creator>Ibharalu, Elijah</creator><creator>Miracle Chibuzor Marcel</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20240301</creationdate><title>Astrometric Measurement of the Double-Star System WDS 09168-3407 B 1118</title><author>Ibharalu, Elijah ; Miracle Chibuzor Marcel</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_29374499293</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Parallax</topic><topic>Position measurement</topic><topic>Separation</topic><toplevel>online_resources</toplevel><creatorcontrib>Ibharalu, Elijah</creatorcontrib><creatorcontrib>Miracle Chibuzor Marcel</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database (Proquest) (PQ_SDU_P3)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Ibharalu, Elijah</au><au>Miracle Chibuzor Marcel</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>Astrometric Measurement of the Double-Star System WDS 09168-3407 B 1118</atitle><jtitle>arXiv.org</jtitle><date>2024-03-01</date><risdate>2024</risdate><eissn>2331-8422</eissn><abstract>We present updated measurements for the position angle and separation of the double-star WDS 09168-3407 B 1118, incorporating data from our observation, Gaia Early Data Release 3 mission, and historical records. Our findings indicate a position angle of 341.4{\deg} and separation of 3.36". Additionally, we utilized parallax and the ratio of proper motion metric (rPM) values to evaluate the potential binarity of the system. Our analysis suggests that the system may be gravitationally bound.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2024-03 |
issn | 2331-8422 |
language | eng |
recordid | cdi_proquest_journals_2937449929 |
source | Publicly Available Content Database (Proquest) (PQ_SDU_P3) |
subjects | Parallax Position measurement Separation |
title | Astrometric Measurement of the Double-Star System WDS 09168-3407 B 1118 |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-27T17%3A31%3A16IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=document&rft.atitle=Astrometric%20Measurement%20of%20the%20Double-Star%20System%20WDS%2009168-3407%20B%201118&rft.jtitle=arXiv.org&rft.au=Ibharalu,%20Elijah&rft.date=2024-03-01&rft.eissn=2331-8422&rft_id=info:doi/&rft_dat=%3Cproquest%3E2937449929%3C/proquest%3E%3Cgrp_id%3Ecdi_FETCH-proquest_journals_29374499293%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2937449929&rft_id=info:pmid/&rfr_iscdi=true |