AstroSat observation of rapid type-I thermonuclear burst from low-mass X-ray binary GX 3+1

• Published in: Journal of astrophysics and astronomy 2022-12, Vol.43 (2), Article 93
• Main Authors: Nath, Ankur, Sarkar, Biplob, Roy, Jayashree, Misra, Ranjeev
• Format: Article
• Language: English
• Subjects: Astronomy; Astrophysics and Astroparticles; Observations and Techniques; Physics; Physics and Astronomy
• ISSN: 0973-7758; 0973-7758
• DOI: 10.1007/s12036-022-09878-9

We report the results of an observation of low-mass X-ray binary GX 3 + 1 with AstroSat’s large area X-ray proportional counter (LAXPC) and soft X-ray telescope (SXT) instruments on-board for the first time. We have detected type-I thermonuclear burst ( ∼ 15 s) present in the LAXPC 20 light curve with a double peak feature at higher energies and our study of the hardness–intensity diagram reveals that the source was in a soft banana state. The pre-burst emission could be described well by a thermally Comptonized model component. The burst spectra is modeled adopting a time-resolved spectroscopic method using a single color blackbody model added to the pre-burst model, to monitor the parametric changes as the burst decays. Based on our time-resolved spectroscopy, we claim that the detected burst is a photospheric radius expansion (PRE) burst. During the PRE phase, the blackbody flux is found to be approximately constant at an averaged value of ∼ 2.56 in 10 - 8 ergs s - 1 cm - 2 units. On the basis of literature survey, we infer that AstroSat/LAXPC 20 has detected a burst from GX 3 + 1 after more than a decade, which is also a PRE one. Utilizing the obtained burst parameters, we provide a new estimation to the source distance, which is ∼ 9.3 ± 0.4 kpc, calculated for an isotropic burst emission. Finally, we discuss and compare our findings with the published literature reports.