Gargi Shaw

Employment

• Tata Institute of Fundamental Research DST- Women scientist
  2018 - Present

Education

• University of Kentucky PhD
  ? - 2005

Projects & Funding

Projects & funding information is unavailable.

Publications (12)

• Hydrodynamic Predictions for the Next Outburst of T Coronae Borealis: It Will Be the Brightest Classical or Recurrent Nova Ever Observed in X-Rays*
  The Astrophysical Journal 2025 DOI: 10.3847/1538-4357/adb8ed
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• Revealing physical properties of a tidal disruption event iPTF16fnl
  Physical Review D 2025 DOI: 10.1103/PhysRevD.111.043041
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• XMM-Newton High-resolution Spectroscopy of EXO 0748–676 after Its Reemergence from a Long Quiescence
  The Astrophysical Journal Letters 2024 DOI: 10.3847/2041-8213/ad9337
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• A phenomenological study of the evolution of shock-induced O i emission lines in the spectrum of nova V2891 Cygni
  Monthly Notices of the Royal Astronomical Society 2024 DOI: 10.1093/mnras/stae1719
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• A Photoionization Model for the Infrared Coronal Line Emission in the Classical Nova V1716 Scorpii
  The Astrophysical Journal 2024 DOI: 10.3847/1538-4357/ad4097
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• Revisiting the Gas-phase Chemical Rate Coefficients at High Temperatures in CLOUDY
  Research Notes of the AAS 2023 DOI: 10.3847/2515-5172/ace9b5
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• Recent Updates of Gas-phase Chemical Reactions and Molecular Lines of SiS in CLOUDY
  Research Notes of the AAS 2023 DOI: 10.3847/2515-5172/acc1ea
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• Recent Updates to the Gas-phase Chemical Reactions and Molecular Lines in CLOUDY: Their Effects on Millimeter and Submillimeter Molecular Line Predictions
  The Astrophysical Journal 2022 DOI: 10.3847/1538-4357/ac7789
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• Photoionization Modeling of the Dusty Nova V1280 Scorpii
  The Astrophysical Journal 2022 DOI: 10.3847/1538-4357/ac36dc
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• Spectroscopic modelling of two high-mass X-ray binaries, Cyg X–3 and 4U 1538–522
  Monthly Notices of the Royal Astronomical Society 2021 DOI: 10.1093/mnras/stab2231
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