2025/08/19 by Mohit Singh Bisht, A. Raj, Bisht, Mohit Singh +11 · 1 voice
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Gamma-ray bursts and supernovae #Astrophysical Phenomena and Observations
paper · doi:10.3847/1538-3881/adfcc6
openalex publication_date 2025/09/15 · openalex created_date 2025/10/10 · openalex updated_date 2026/06/11
Abstract We present a detailed spectrophotometric study of nova LMCN 2009-05a, located in the Large Magellanic Cloud (LMC). Photometric observations reveal a dust dip in the optical light curve, classifying it as a D-class nova. Light curve analysis yields t 2 and t 3 decline times of approximately 46 and 80 days, respectively, placing the nova in the category of moderately fast novae. Spectroscopic observations cover multiple phases, including pre-maximum, early decline, and nebular. The spectra are initially dominated by hydrogen Balmer and Fe II lines with P-Cygni profiles, which later transition into pure emission. During the optical minimum, a discrete absorption feature was observed in the H α and [O I ] line profiles. The physical and chemical properties during the early decline and nebular phases were analyzed using the photoionization code CLOUDY. Dust temperature, mass, and grain size were estimated through spectral energy distribution fitting to the WISE data. On day 395 post-outburst, we estimate the dust temperature to be approximately 700 K. Additionally, we examined the correlation between dust condensation time ( t cond ) and t 2 for LMC novae, finding a trend consistent with previous studies of Galactic novae.