activity
20242026
collaborators

7 papers

astro-ph.SR2026

Large Magellanic Cloud Globular Clusters in the Near-infrared. I. RR Lyrae in Reticulum

Anupam Bhardwaj, Susmita Das, Prashant Nishad +10

Reticulum is an old, metal-poor, and sparsely populated globular cluster in the outer regions of the Large Magellanic Cloud (LMC) and hosts a rich population of RR Lyrae stars. Bei…

astro-ph.SR2026

Self-Consistent Nonlinear Classical Cepheid Pulsations During Stellar Evolution with MESA

Ebraheem Farag, Earl P. Bellinger, Philip Mocz +5

We extend the time-dependent convection treatment in \code{MESA} by introducing eddy-viscous damping. This software change brings \code{MESA-TDC} into closer alignment with the rad…

astro-ph.SR2026

The effect of metallicity on the Leavitt Law using phase-dependent properties of classical Cepheids

Gautam Bhuyan, Shashi Kanbur, Sukanta Deb +5

The absolute calibration of period-luminosity (PL) relations of Cepheids in the Milky Way (MW) and its nearby galaxies has been a cornerstone in determining extragalactic distances…

astro-ph.SR2025

The light curve model fitting of LMC Cepheids: MESA-RSP versus Stellingwerf's code predictions

M. Deka, M. Marconi, R. Molinaro +9

A major challenge in modeling classical Cepheids is the treatment of convection, particularly its complex interplay with pulsation. This inherently three-dimensional process is typ…

astro-ph.GA2025

Multiwavelength study of observed and predicted pulsation properties of First overtone Cepheids in the Magellanic Clouds

Kerdaris Kurbah, Shashi M. Kanbur, Sukanta Deb +4

We present a detailed analysis of the light curves and pulsation properties of First Overtone (FO) Cepheids in the Magellanic Clouds (MCs) obtained using observations and predictio…

astro-ph.SR2025

A theoretical framework for BL Her stars IV. New period-luminosity relations in the Rubin-LSST filters

Susmita Das, László Molnár, Róbert Szabó +5

We present new theoretical light curves in the Rubin-LSST filters for a fine grid of BL Her models computed using MESA-RSP. We also derive new theoretical period-luminosity (PL) an…