Proceedings of THE 5th INTERNATIONAL CONFERENCE OF HYOJEONG ACADEMY (2025.02)바로가기
페이지
pp.81-86
저자
Ivan Chelovekov
언어
영어(ENG)
URL
https://www.earticle.net/Article/A489348
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4,000원
원문정보
초록
영어
Low mass X-ray binaries are binary star systems, consisting of a late type main sequence star and a compact object. This class of objects is known to emit regular X-ray flares on the time scales of years to decades. In our work we present an energy balance stage model for such a behavior and apply it to the case of IGR J17498-2921 2023 Apr. flare. We present the results of our analysis of NUSTAR and Spektr-RG/ART-XC observations of the source. Each of the satellites detected 2 type I X-ray bursts from the source, which let us determine burst recurrence period during flare activity, estimate its possible value during the quiescence period and gave a hint on accreted material composition. Comparatively low burst duration witnesses of a H poor accreted material and so a highly evolved optical companion star. Burst spectra were well fitted with absorbed thermal radiation model, while persistent radiation spectra also required a hot corona, accretion disk and reflection of coronal radiation from the disk components to be added to the model.
목차
Abstract 1. Introduction 1.1. Observations and data analysis 2. Results 2.1. The model References
Journal of Hyojeong Academia aims to serve as a global platform where researchers and scholars of various disciplines can contribute ideas for our sustainable global community of Co‐existence, Co‐prosperity, and Co‐righteousness. The journal is a multidisciplinary, open‐access, internationally peer‐reviewed
academic journal, and it invites all areas of research conducted in the spirit of post materialism including studies centering on God, studies unifying religions and
sciences, and studies on all aspects of Co‐existence, Co‐prosperity, and Co‐righteousness.
간행물
간행물명
선문효정학술연구회 학술대회 프로시딩
간기
반년간
수록기간
2023~2026
십진분류
KDC 238DDC 289
이 권호 내 다른 논문 / 선문효정학술연구회 학술대회 프로시딩 Proceedings of THE 5th INTERNATIONAL CONFERENCE OF HYOJEONG ACADEMY