تقرير
Study of the q diagram in GX 339-4
| العنوان: | Study of the q diagram in GX 339-4 |
|---|---|
| المؤلفون: | Agarwal, Sanyukta, Yadav, J. S. |
| سنة النشر: | 2022 |
| المجموعة: | Astrophysics |
| مصطلحات موضوعية: | Astrophysics - High Energy Astrophysical Phenomena |
| الوصف: | Black hole X-ray binary (BHXB) GX 339-4 produces the most frequent X-ray outbursts (every 2-4 years) among known X-ray binary sources in our galaxy. Here we present the study of the evolution of GX 339-4 over the years of observations using the Hardness Intensity Diagram (HID), i.e., the q diagram. We present an analysis of two outbursts of the source observed by the Monitor of All-sky X-ray Image (MAXI) telescope aboard the International Space Station (ISS). Comment: 4 pages, 4 figures |
| نوع الوثيقة: | Working Paper |
| URL الوصول: | http://arxiv.org/abs/2209.07166 |
| رقم الأكسشن: | edsarx.2209.07166 |
| قاعدة البيانات: | arXiv |
| الوصف غير متاح. |