V1082 Sgr is a cataclysmic variable with accretion luminosity above 1034erg s−1, indicating a mass transfer rate above 10−9M⊙yr−1. However, its K type companion was suggested to be under-filling its Roche lobe (RL), making the high mass transfer rate a mystery. In this work we propose a possible model to explain this discrepancy. The system is proposed to be an intermediate polar, with its K type companion filling its RL. The mass of the white dwarf star is evaluated to be 0.77±0.11M⊙ from both X-ray continuum fitting and Fe line flux ratio measurements. We make numerical simulations to search for the possible progenitors of the system. The results show that a binary with an initial 1.5--2.5M⊙ companion in a 1--2 day orbit (or an initial 1.0--1.4M⊙ companion in a 3.2--4.1 day orbit) may naturally evolve to a cataclysmic variable with a ∼0.55±0.11M⊙, Roche-lobe filling companion in a 0.86 day orbit. The effective temperature of the donor star, the mass transfer rate, and the derived V band magnitude are all consistent with previous observations.
@article{arxiv.1908.10519,
title = {V1082-Sgr: A magnetic cataclysmic variable with a lobe-filling companion star},
author = {Xiao-jie Xu and Yong Shao and Xiang-dong Li},
journal= {arXiv preprint arXiv:1908.10519},
year = {2019}
}