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    <name>Article</name>
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              <text>Broad-band mHz QPOs and spectral study of LMC X-4 with AstroSat</text>
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              <text>accretion, accretion discs; pulsars: general; stars: neutron; X-rays: binaries; X-rays: individual: LMC X-4</text>
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              <text>We report the results of broad-band timing and spectral analysis of data from an AstroSat observation of the high-mass X-ray binary LMC X-4. The Large Area X-ray Proportional Counter (LAXPC) and Soft X-ray Telescope (SXT) instruments onboard the AstroSat observed the source in 2016 August. A complete X-ray eclipse was detected with the LAXPC. The 340 keV power density spectrum showed the presence of coherent pulsations along with a ?26 mHz quasi-periodic oscillation feature. The spectral properties of LMC X-4 were derived from a joint analysis of the SXT and LAXPC spectral data. The 0.525 keV persistent spectrum comprised of an absorbed high-energy cut-off power law with photon index of ? ? 0.8 and cut-off at ?16 keV, a soft thermal component with kTBB ? 0.14 keV, and Gaussian components corresponding to Fe K?, Ne IX, and Ne X emission lines. Assuming a source distance of 50 kpc, we determined 0.525 keV luminosity to be ?2 1038 erg s?1  2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.</text>
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          <name>Creator</name>
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              <text>Sharma R.; Jain C.; Rikame K.; Paul B.</text>
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              <text>Monthly Notices of the Royal Astronomical Society, Vol-519, No. 2, pp. 1764-1770.</text>
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              <text>Oxford University Press</text>
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              <text>2023-01-01</text>
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              <text>&lt;a href="https://doi.org/10.1093/mnras/stac3572" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1093/mnras/stac3572&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85159153408&amp;amp;doi=10.1093%2Fmnras%2Fstac3572&amp;amp;partnerID=40&amp;amp;md5=79bfd819ac1d92b7ac6ce6bbfa9012f1" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85159153408&amp;amp;doi=10.1093%2fmnras%2fstac3572&amp;amp;partnerID=40&amp;amp;md5=79bfd819ac1d92b7ac6ce6bbfa9012f1&lt;/a&gt;</text>
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              <text>All Open Access; Green Open Access</text>
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              <text>ISSN: 358711; CODEN: MNRAA</text>
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              <text>Online</text>
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              <text>English</text>
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              <text>Sharma R., Raman Research Institute, C.V. Raman Avenue, Sadashivanagar, Karnataka, Bengaluru, 560080, India; Jain C., Hansraj College, University of Delhi, Delhi, 110007, India; Rikame K., Raman Research Institute, C.V. Raman Avenue, Sadashivanagar, Karnataka, Bengaluru, 560080, India, Department of Physics and Electronics, CHRIST (Deemed to be University), Karnataka, Bengaluru, 560029, India; Paul B., Raman Research Institute, C.V. Raman Avenue, Sadashivanagar, Karnataka, Bengaluru, 560080, India</text>
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