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            <name>Title</name>
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    <name>Article</name>
    <description>Faculty Publications -Articles</description>
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          <name>Title</name>
          <description>A name given to the resource</description>
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              <text>Discovery of an M-type companion to the Herbig Ae Star V1787 Ori</text>
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          <name>Subject</name>
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              <text>binaries: visual; stars: pre-main-sequence; stars: variables: T Tauri, Herbig Ae/Be</text>
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          <name>Description</name>
          <description>An account of the resource</description>
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              <text>The intermediate-mass Herbig Ae star V1787 Ori is a member of the L1641 star-forming region in the Orion A molecular cloud. We report the detection of an M-type companion to V1787 Ori at a projected separation of 6.66 arcsec (corresponding to 2577 au), from the analysis of VLT/NACO adaptive optics Ks-band image. Using astrometric data from Gaia DR2, we show that V1787 Ori A and B share similar distance (d ?387 pc) and proper motion, indicating that they are physically associated. We estimate the spectral type of V1787 Ori B to be M5  2 from colour-spectral type calibration tables and template matching using SpeX spectral library. By fitting PARSEC models in the Pan-STARRS colour-magnitude diagram, we find that V1787 Ori B has an age of 8.1$^{+1.7}_{-1.5}$ Myr and a mass of 0.39$^{+0.02}_{-0.05}$ M. We show that V1787 Ori is a pre-main-sequence wide binary system with a mass ratio of 0.23. Such a low-mass ratio system is rarely identified in Herbig Ae/Be binary systems. We conclude this work with a discussion on possible mechanisms for the formation of V1787 Ori wide binary system.   2020 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.</text>
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              <text>Arun R.; Mathew B.; Rengaswamy S.; Manoj P.; Narang M.; Kartha S.S.; Maheshwar G.</text>
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              <text>Monthly Notices of the Royal Astronomical Society, Vol-501, No. 1, pp. 1243-1252.</text>
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              <text>Oxford University Press</text>
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          <name>Date</name>
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              <text>2021-01-01</text>
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          <name>Identifier</name>
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              <text>&lt;a href="https://doi.org/10.1093/mnras/staa3652" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1093/mnras/staa3652&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85100356179&amp;amp;doi=10.1093%2Fmnras%2Fstaa3652&amp;amp;partnerID=40&amp;amp;md5=a1decf917f96ac41f60abeda90c6c772" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85100356179&amp;amp;doi=10.1093%2fmnras%2fstaa3652&amp;amp;partnerID=40&amp;amp;md5=a1decf917f96ac41f60abeda90c6c772&lt;/a&gt;</text>
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          <name>Rights</name>
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              <text>All Open Access; Green Open Access</text>
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          <name>Relation</name>
          <description>A related resource</description>
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              <text>ISSN: 358711; CODEN: MNRAA</text>
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          <name>Format</name>
          <description>The file format, physical medium, or dimensions of the resource</description>
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              <text>Online</text>
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          <name>Language</name>
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              <text>English</text>
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              <text>Article</text>
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              <text>Arun R., Department of Physics and Electronics, Christ Deemed to Be University, Bangalore, 560029, India; Mathew B., Department of Physics and Electronics, Christ Deemed to Be University, Bangalore, 560029, India; Rengaswamy S., Department of Physics and Electronics, Christ Deemed to Be University, Bangalore, 560029, India; Manoj P., Department of Physics and Electronics, Christ Deemed to Be University, Bangalore, 560029, India; Narang M., Department of Physics and Electronics, Christ Deemed to Be University, Bangalore, 560029, India; Kartha S.S., Department of Physics and Electronics, Christ Deemed to Be University, Bangalore, 560029, India; Maheshwar G., Department of Physics and Electronics, Christ Deemed to Be University, Bangalore, 560029, India</text>
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