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pro vyhledávání: '"Mukherjee U"'
Publikováno v:
Lung Cancer: Targets and Therapy, Vol Volume 13, Pp 53-66 (2022)
Joséphine Carpentier,1 Iuliia Pavlyk,1 Uma Mukherjee,2 Peter E Hall,2 Peter W Szlosarek1,2 1Centre for Cancer Biomarkers and Biotherapeutics, Barts Cancer Institute, Queen Mary University of London, London, EC1M 6BQ, UK; 2Department of Medical Oncol
Externí odkaz:
https://doaj.org/article/c409671b94c34c679f64974823707674
Autor:
Reddy, B. Deepak, Kumar, Birendra, Sahni, Sangita, Yashaswini, G., Karthik, Somala, Reddy, M. S. Sai, Kumar, Rajeev, Mukherjee, U., Krishna, K. Sai
Publikováno v:
Scientific Reports; 5/31/2024, Vol. 14 Issue 1, p1-16, 16p
Akademický článek
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We report here results from detailed timing and spectral studies of the high mass X-ray binary pulsar 4U~1538--52 over several binary periods using observations made with the Rossi X-ray Timing Explorer (RXTE) and BeppoSAX satellites. Pulse timing an
Externí odkaz:
http://arxiv.org/abs/astro-ph/0702142
We have investigated the Quasi Periodic Oscillation (QPO) properties of the transient accreting X-ray pulsar XTE J1858+034 during the second outburst of this source in April-May 2004. We have used observations made with the Proportional Counter Array
Externí odkaz:
http://arxiv.org/abs/astro-ph/0602559
Autor:
Mukherjee, U., Paul, B.
Here we report the spectral characteristics of the high and low states of the pulsar 4U~0114+65 and examine the change in the parameters of the spectral model. A power law and a photoelectric absorption by material along the line of sight together wi
Externí odkaz:
http://arxiv.org/abs/astro-ph/0602558
Autor:
Mukherjee, U., Paul, B.
High Mass X-ray Binary Pulsars (HMXBP), in which the companion star is a source of supersonic stellar wind, provide a laboratory to probe the velocity and density profile of such winds. Here, we have measured the variation of the absorption column de
Externí odkaz:
http://arxiv.org/abs/astro-ph/0512095
We report here discovery of the existence of two different accretion modes in the high mass X-ray binary pulsar Cen X-3 during its high states. The multiband X-ray light curves of Cen X-3 lasting for more than 3400 days obtained with the All Sky Moni
Externí odkaz:
http://arxiv.org/abs/astro-ph/0509097
Publikováno v:
Astrophys.J. 627 (2005) 915-919
We present here high resolution X-ray spectrum of the accreting binary X-ray pulsar GX 1+4 obtained with the High Energy Transmission Grating (HETG) instrument of the Chandra X-ray Observatory. This was supplemented by a simultaneous observation with
Externí odkaz:
http://arxiv.org/abs/astro-ph/0503530
Autor:
Mukherjee, U., Paul, B.
We present the timing and spectral properties of the transient Be/X-ray binary pulsar 3A 0535+262 during quiescence using three observations with the narrow field imaging instruments (NFI) of BeppoSAX. Assuming a distance of 2 kpc for this system, th
Externí odkaz:
http://arxiv.org/abs/physics/0410255