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            <name>Title</name>
            <description>A name given to the resource</description>
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                <text>Faculty Publications</text>
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    <name>Article</name>
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      <name>Dublin Core</name>
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          <name>Creator</name>
          <description>An entity primarily responsible for making the resource</description>
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            <elementText elementTextId="209992">
              <text>Purandardas, Meenakshi; Dutta, Debasish; Goswami, Aruna; Kartha, Sreeja S.</text>
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          <name>Title</name>
          <description>A name given to the resource</description>
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            <elementText elementTextId="209993">
              <text>High-resolution spectral analysis of three high-latitude carbon stars</text>
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          <name>Date</name>
          <description>A point or period of time associated with an event in the lifecycle of the resource</description>
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            <elementText elementTextId="209994">
              <text>01-01-2025</text>
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          <name>Source</name>
          <description>A related resource from which the described resource is derived</description>
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              <text>Publications of the Astronomical Society of Australia;Volume;42;Issue;;Article No.;e047;</text>
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          <name>Identifier</name>
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              <text>&lt;a href="https://doi.org/10.1017/pasa.2025.32" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1017/pasa.2025.32&lt;/a&gt; &lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/pages/publications/105004860127?origin=resultslist" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/pages/publications/105004860127?origin=resultslist&lt;/a&gt;</text>
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              <text>Purandardas M., Department of Physics and Electronics, CHRIST (Deemed to Be University), Bangalore, India; Dutta D., Indian Institute of Astrophysics, Koramangala, Bangalore, India, Indian Institute of Technology, Kanjikode, Kerala, Palakkad, India; Goswami A., Indian Institute of Astrophysics, Koramangala, Bangalore, India, Institute of Frontier Science and Application, Bangalore, India; Kartha S.S., Department of Physics and Electronics, CHRIST (Deemed to Be University), Bangalore, India</text>
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              <text>We present the results of a detailed high-resolution spectroscopic analysis (SUBARU/HDS spectra, R 50 000) of three faint high-latitude carbon stars HE 1104 0957, HE 1205 0521, and HE 1244 3036. Our estimated metallicity for these objects is 2.96, 2.63, and 2.49, respectively. The surface chemical compositions of the objects are found to be characterised by enhanced carbon and heavy elements, such as Y, Ba, La, and Ce. Using the classification criteria for carbon-enhanced metal-poor (CEMP) stars the objects HE 1104 0957 and HE 1205 0521 could not be classified into any known CEMP sub-classes, whereas the object HE 1244 3036 is found to be likely a CEMP-s star. The observed abundance patterns in HE 1244 3036 are also found to match well with the yields of a 2 M AGB star with [Fe/H] = 2.50. Although our kinematic analysis indicates that the objects belong to the halo population, the elemental abundance ratios of HE 1104 0957 and HE 1205 0521 do not match well with those of typical halo objects. Estimated elemental abundances are presented, and kinematic properties of the stars are discussed.   The Author(s), 2025.</text>
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          <name>Subject</name>
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              <text>Stars: abundances; stars: atmospheres; stars: carbon stars; stars: metal-poor</text>
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          <name>Publisher</name>
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              <text>Cambridge University Press</text>
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              <text>ISSN: 13233580;</text>
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              <text>All Open Access; Hybrid Gold Open Access</text>
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          <name>Format</name>
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              <text>online</text>
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