Statistical Survey for the Physical Characteristic of Near Contact Binary(NCBs)

The absolute dimensions and orbital elements of 66 near contact binaries, collected from literatures, have been analyzed to investigate the physical characteristics of the near contact binaries as well as co-relations among physical parameters. The relationship between the mass ratio and luminosity...

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Main Author: Kyu-Dong Oh
Format: Article
Language:English
Published: The Korean Space Science Society 2005-09-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2005/v22n3/OJOOBS_2005_v22n3_233.pdf
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author Kyu-Dong Oh
author_facet Kyu-Dong Oh
author_sort Kyu-Dong Oh
collection DOAJ
description The absolute dimensions and orbital elements of 66 near contact binaries, collected from literatures, have been analyzed to investigate the physical characteristics of the near contact binaries as well as co-relations among physical parameters. The relationship between the mass ratio and luminosity ratio of the near contact binary systems have been obtained as a L2/L1 ≈ (M2/M1)^1.45, which is similar to that of the early type contact binary system. The physical parameters of the near contact binaries show that the difference in mass, radius, luminosity and temperature between the primary and the secondary components for the F type NCBs are smaller than those for the A type NCBs. In H-R diagram, the components of the A types are located closer to the terminal age main sequence than those of the F types.
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spelling doaj.art-adb0640c15ba4a85ba0de5f97576e9dd2024-02-02T21:55:04ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14092005-09-0122323324210.5140/JASS.2005.22.3.233Statistical Survey for the Physical Characteristic of Near Contact Binary(NCBs)Kyu-Dong Oh0Department of Earth Science Education, Chonnam National University, Kwangju 500-757, KoreaThe absolute dimensions and orbital elements of 66 near contact binaries, collected from literatures, have been analyzed to investigate the physical characteristics of the near contact binaries as well as co-relations among physical parameters. The relationship between the mass ratio and luminosity ratio of the near contact binary systems have been obtained as a L2/L1 ≈ (M2/M1)^1.45, which is similar to that of the early type contact binary system. The physical parameters of the near contact binaries show that the difference in mass, radius, luminosity and temperature between the primary and the secondary components for the F type NCBs are smaller than those for the A type NCBs. In H-R diagram, the components of the A types are located closer to the terminal age main sequence than those of the F types.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2005/v22n3/OJOOBS_2005_v22n3_233.pdfbinary starnear contact binaryH-R diagram of near contact binary
spellingShingle Kyu-Dong Oh
Statistical Survey for the Physical Characteristic of Near Contact Binary(NCBs)
Journal of Astronomy and Space Sciences
binary star
near contact binary
H-R diagram of near contact binary
title Statistical Survey for the Physical Characteristic of Near Contact Binary(NCBs)
title_full Statistical Survey for the Physical Characteristic of Near Contact Binary(NCBs)
title_fullStr Statistical Survey for the Physical Characteristic of Near Contact Binary(NCBs)
title_full_unstemmed Statistical Survey for the Physical Characteristic of Near Contact Binary(NCBs)
title_short Statistical Survey for the Physical Characteristic of Near Contact Binary(NCBs)
title_sort statistical survey for the physical characteristic of near contact binary ncbs
topic binary star
near contact binary
H-R diagram of near contact binary
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2005/v22n3/OJOOBS_2005_v22n3_233.pdf
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