| Name: Sanjit Pal |
| Affiliation: Raman Research Institute |
| Conference ID: ASI2026_343 |
| Title: Emission line diagnostics of evolving supernova remnants |
| Abstract Type: Poster |
| Abstract Category: Stars, Interstellar Medium, and Astrochemistry in Milky Way |
| Author(s) and Co-Author(s) with Affiliation: Sanjit Pal(Raman Research Institute), Kartick Sarkar(Raman Research Institute) |
| Abstract: This work investigates the synthetic observations of supernova remnant simulations performed using the hydrodynamic code, PLUTO. The numerical simulations include a dynamically evolving non-equilibrium ionization network and a frequency-dependent radiation transfer coupled to each other and to the hydrodynamics. The work aims to show the time-dependent relation of the emission line ratios from an SNR on the classical Baldwin, Phillips & Terlevich (BPT) diagram. We present a comparison model with various initial conditions and parameters, such as varying number densities, metallicities, etc., as well as a direct comparison to observational surveys.
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