Scholarlink

Abstract <p>A high-precision algorithm for interpreting transit light curves in the model of an eclipsing classical binary star–exoplanet system for interpretation moving from the eccentricity (<InlineEquation ID="IEq1"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11444_2025_1687_Article_IEq1.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="11" /> </InlineMediaObject> <EquationSource Format="TEX">\(e\)</EquationSource> <!--AstEng2570184Abubekerov-m1--> </InlineEquation>)–periastron longitude (<InlineEquation ID="IEq2"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11444_2025_1687_Article_IEq2.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="14" /> </InlineMediaObject> <EquationSource Format="TEX">\(\omega \)</EquationSource> <!--AstEng2570184Abubekerov-m2--> </InlineEquation>) variables to the (<InlineEquation ID="IEq3"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11444_2025_1687_Article_IEq3.gif" Format="GIF" Height="17" Rendition="HTML" Resolution="72" Type="Linedraw" Width="106" /> </InlineMediaObject> <EquationSource Format="TEX">\(e\cos \omega ,\;{\kern 1pt} e\sin \omega \)</EquationSource> <!--AstEng2570184Abubekerov-m3--> </InlineEquation>) eccentricity components has been improved. The possibilities of interpretation by eccentricity components have been studied. It has been shown that the dependence of the minimum’s shape on <InlineEquation ID="IEq4"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11444_2025_1687_Article_IEq4.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="47" /> </InlineMediaObject> <EquationSource Format="TEX">\(e\sin \omega \)</EquationSource> <!--AstEng2570184Abubekerov-m4--> </InlineEquation> alone is clearly expressed at small <i>e</i> values and weakens with increasing <InlineEquation ID="IEq5"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11444_2025_1687_Article_IEq1.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="11" /> </InlineMediaObject> <EquationSource Format="TEX">\(e\)</EquationSource> <!--AstEng2570184Abubekerov-m5--> </InlineEquation>. The linear correlation between the radius value, which is characteristic of any <i>e</i> values, has been shown.</p>

错误：搜索内容不能为空，请输入英文关键词
错误：关键词超出字数限制，请精简
高级检索

Aspects of Optimization of the Transit Light Curve of the Binary System with a Single Minimum by the Eccentricity Components

  • 期刊论文

  • 发表日期：

    2025年6月1日

查看全文
  • M. K. Abubekerov,
  • N. Yu. Gostev

摘要

Abstract

A high-precision algorithm for interpreting transit light curves in the model of an eclipsing classical binary star–exoplanet system for interpretation moving from the eccentricity ( \(e\) )–periastron longitude ( \(\omega \) ) variables to the ( \(e\cos \omega ,\;{\kern 1pt} e\sin \omega \) ) eccentricity components has been improved. The possibilities of interpretation by eccentricity components have been studied. It has been shown that the dependence of the minimum’s shape on \(e\sin \omega \) alone is clearly expressed at small e values and weakens with increasing \(e\) . The linear correlation between the radius value, which is characteristic of any e values, has been shown.