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DC Field | Value | Language |
---|---|---|
dc.contributor.author | Sarkar, Tamal | - |
dc.date.accessioned | 2024-03-31T10:51:58Z | - |
dc.date.available | 2024-03-31T10:51:58Z | - |
dc.date.issued | 2024-03 | - |
dc.identifier.issn | XXXX-XXXX (Online) | - |
dc.identifier.issn | XXXX-XXXX (Print); | - |
dc.identifier.uri | http://ir.nbu.ac.in/handle/123456789/5180 | - |
dc.description.abstract | LSI + 61o 303 is a high-mass X-ray binary consisting of a low-mass [M (1 - 4)M ] compact object orbiting around an early type B0 Ve star along an eccentric e = 0:7 orbit. It along with LS5039 are the only two known gamma-ray binary detected in the TeV band. Despite extensive observations the nature of this source, particularly whether it is a pulsar or a black hole (microquasar) system, is not clear. The mechanisms that lead to the multi-wavelength behavior are also uncertain. Recent approach to the study of LSI + 61o 303 has been to focus on possible correlated variability. There was an early indication that there is a correlation between the X-ray and TeV emission at the time where the latter was measurable. In a more recent observation, however, such a feature has not been found. In this work, we study the spectral variability of LSI + 61o 303 using four observations between 2001 to 2007 of XMM - Newton available from NASA archive and examine the correlation between low energy range and high energy part. | en_US |
dc.language.iso | en | en_US |
dc.publisher | University of North Bengal | en_US |
dc.subject | Spectral variability | en_US |
dc.subject | Orbital profiles of TeV Binary LSI + 61o 303 | en_US |
dc.subject | X-Ray window | en_US |
dc.subject | using XMM - Newton Observations | en_US |
dc.title | Spectral variability in the orbital profiles of TeV Binary LSI + 61o 303 in X-Ray window using XMM - Newton Observations | en_US |
dc.title.alternative | J. Phys. Res. Edu., Vol. 2, March 2024, pp 80-87 | en_US |
dc.type | Article | en_US |
Appears in Collections: | Journal of Physics Research and Education, Vol. 2 March, 2024 |
Files in This Item:
File | Description | Size | Format | |
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Spectral variability in the orbital profiles of TeV Binary LSI + 61o 303 in X-Ray window using XMN_Newton Observations_08.pdf | Spectral variability in the orbital profiles of TeV Binary LSI + 61o 303 in X-Ray window using XMM Newton Observations | 717.76 kB | Adobe PDF | View/Open |
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