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| Language: | English |
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2025
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| Online Access: | https://doi.org/10.5281/zenodo.14601214 |
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| author | Ashok Mondal Nayab Gauhar |
| author_facet | Ashok Mondal Nayab Gauhar |
| contents | <p><sup><span>1</span></sup><span>Ashok Mondal,<sup>2</sup></span>Nayab Gauhar</p> <p><em><sup><span>1</span></sup></em><em><span>Department of Applied Science and Humanities, Haldia Institute of Technology, Haldia, Purba Medinipur, West Bengal</span></em></p> <p><em><sup><span>2,</span></sup><span>Department. of <span> </span>Computer Science <span> </span>Engineering, Haldia Institute of Technology, Haldia, Purba Medinipur, West Bengal</span></em></p> <p><strong><span>ABSTRACT</span></strong></p> <p><em><span><span>This study investigates the temporal evolution of X-ray transients, focusing on the relationship between the total mass of these systems and the increasing number of stars formed after a starburst event. </span><span><span> </span>The total binary mass considered is </span><span> </span><span>and the analysis spans the first 20 million years after the burst. The simulations includes transient sources accreting neutron stars paired with Be-type stars. </span><span>By analyzing data across different time intervals, we observe a consistent trend where the total mass of X-ray transients decreases over time, while the number of stars increases. This inverse relationship highlights the dynamic interplay between accretion processes, mass loss mechanisms, and environmental factors, such as star formation history and local stellar density. Early stages of evolution show relatively stable mass retention, suggesting efficient accretion mechanisms, whereas later stages exhibit significant mass depletion, likely driven by material exhaustion or outflow processes. These findings provide valuable insights into the lifecycle of X-ray transient systems and their connection to broader astrophysical phenomena, including accretion disk dynamics and high-energy emissions. The results emphasize the importance of continued observations and high-resolution simulations to unravel the complex processes governing the evolution of these transient systems</span></span></em></p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_14601214 |
| institution | Zenodo |
| language | eng |
| publishDate | 2025 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Evolution of total mass of X-ray transients over different time intervals Ashok Mondal Nayab Gauhar X-ray Sources Star burst Initial mass function <p><sup><span>1</span></sup><span>Ashok Mondal,<sup>2</sup></span>Nayab Gauhar</p> <p><em><sup><span>1</span></sup></em><em><span>Department of Applied Science and Humanities, Haldia Institute of Technology, Haldia, Purba Medinipur, West Bengal</span></em></p> <p><em><sup><span>2,</span></sup><span>Department. of <span> </span>Computer Science <span> </span>Engineering, Haldia Institute of Technology, Haldia, Purba Medinipur, West Bengal</span></em></p> <p><strong><span>ABSTRACT</span></strong></p> <p><em><span><span>This study investigates the temporal evolution of X-ray transients, focusing on the relationship between the total mass of these systems and the increasing number of stars formed after a starburst event. </span><span><span> </span>The total binary mass considered is </span><span> </span><span>and the analysis spans the first 20 million years after the burst. The simulations includes transient sources accreting neutron stars paired with Be-type stars. </span><span>By analyzing data across different time intervals, we observe a consistent trend where the total mass of X-ray transients decreases over time, while the number of stars increases. This inverse relationship highlights the dynamic interplay between accretion processes, mass loss mechanisms, and environmental factors, such as star formation history and local stellar density. Early stages of evolution show relatively stable mass retention, suggesting efficient accretion mechanisms, whereas later stages exhibit significant mass depletion, likely driven by material exhaustion or outflow processes. These findings provide valuable insights into the lifecycle of X-ray transient systems and their connection to broader astrophysical phenomena, including accretion disk dynamics and high-energy emissions. The results emphasize the importance of continued observations and high-resolution simulations to unravel the complex processes governing the evolution of these transient systems</span></span></em></p> |
| title | Evolution of total mass of X-ray transients over different time intervals |
| topic | X-ray Sources Star burst Initial mass function |
| url | https://doi.org/10.5281/zenodo.14601214 |