Zobrazeno 1 - 10
of 222
pro vyhledávání: '"Jithesh, V."'
Autor:
Ezhikode, Savithri H., Anilkumar, Hema, Arun, R., Mathew, Blesson, Jithesh, V., Bhattacharyya, Suman, Nedhath, Sneha, Cysil, T. B., Muneer, S., Kartha, Sreeja S., S, Pramod Kumar
Weak-line T Tauri stars (WTTS) exhibit X-ray flares, likely resulting from magnetic reconnection that heats the stellar plasma to very high temperatures. These flares are difficult to identify through targeted observations. Here, we report the serend
Externí odkaz:
http://arxiv.org/abs/2410.16241
Autor:
Anilkumar, Hema, Mathew, Blesson, Jithesh, V., Kartha, Sreeja S., Manoj, P., Narang, Mayank, Chavali, Mahathi
Herbig Ae/Be (HAeBe) stars are intermediate-mass pre-main sequence stars, characterized by infrared excess and emission lines. They are observed to emit X-rays, whose origin is a matter of discussion and not settled yet. X-ray emission is not expecte
Externí odkaz:
http://arxiv.org/abs/2404.03403
In eclipsing X-ray binary systems, the direct X-ray emission is blocked by the companion star during the eclipse. We observe only reprocessed emission that contains clues about the environment of the compact object and its chemical composition, ioniz
Externí odkaz:
http://arxiv.org/abs/2403.05936
Since its discovery in 1992, GRS 1915+105 has been among the brightest sources in the X-ray sky. However, in early 2018, it dimmed significantly and has stayed in this faint state ever since. We report on AstroSat and NuSTAR observation of GRS 1915+1
Externí odkaz:
http://arxiv.org/abs/2402.06569
Autor:
Raiteri, C. M., Villata, M., Carnerero, M. I., Savchenko, S. S., Kurtanidze, S. O., Vlasyuk, V. V., Marchini, A., Matsumoto, K., Lorey, C., Joner, M. D., Gazeas, K., Carosati, D., Mirzaqulov, D. O., Pulido, J. A. Acosta, Agudo, I., Bachev, R., Benítez, E., Borman, G. A., Calcidese, P., Chen, W. P., Damljanovic, G., Ehgamberdiev, S. A., Elsässer, D., Feige, M., Frasca, A., Gaur, H., Grishina, T. S., Gupta, A. C., Hiriart, D., Holland, M., Horst, B., Ibryamov, S., Ivanidze, R. Z., Jensen, J., Jithesh, V., Jovanovic, M. D., Kiehlmann, S., Kimeridze, G. N., Kishore, S., Kopatskaya, E. N., Kurtanidze, O. M., Larionova, E. G., Lin, H. C., Mannheim, K., Marinelli, C., Reyes, J. Moreira, Morozova, D. A., Nikolashvili, M. G., Reinhart, D., Romanov, F. D., Semkov, E., Seufert, J., Shishkina, E. V., Sigua, L. A., Skalidis, R., Spiridonova, O. I., Stojanovic, M., Strigachev, A., Troitskaya, Y. V., Troitskiy, I. S., Tsai, A., Vasilyev, A. A., Vince, O., Vrontaki, K., Wani, K., Watts, D., Zhovtan, A. V.
In 2022 the BL Lac object S4 0954+65 underwent a major variability phase, reaching its historical maximum brightness in the optical and $\gamma$-ray bands. We present optical photometric and polarimetric data acquired by the Whole Earth Blazar Telesc
Externí odkaz:
http://arxiv.org/abs/2310.11108
Autor:
Barua, Samuzal, Adegoke, Oluwashina K., Misra, Ranjeev, Pawar, Pramod, Jithesh, V., Medhi, Biman J.
Publikováno v:
APJ, 958, 46, 2023
Correlated variability between coronal X-rays and disc optical/UV photons provides a very useful diagnostic of the interplay between the different regions around an active galactic nucleus (AGN) and how they interact. AGN that reveal strong X-ray ref
Externí odkaz:
http://arxiv.org/abs/2308.11552
Autor:
Mondal, Santanu, Jithesh, V.
We present the X-ray spectral and temporal analysis of the black hole X-ray transient Swift J1658.2--4242 observed by {\it AstroSat}. Three epochs of data have been analysed using the JeTCAF model to estimate the mass accretion rates and to understan
Externí odkaz:
http://arxiv.org/abs/2304.04422
Correlated variability of the reflection fraction with the X-ray flux and spectral index for Mkn 478
Publikováno v:
MNRAS, 517, 801-807, 2022
The X-ray spectrum of Mkn 478 is known to be dominated by a strong soft excess which can be described using relativistic blurred reflection. Using observations from {\it XMM-Newton}, {\it AstroSat} and {\it Swift}, we show that for the long-term ($\s
Externí odkaz:
http://arxiv.org/abs/2209.08969
Publikováno v:
APJ,939,80,2022
We present an extensive study on the X-ray intraday variability of ten TeV-emitting high synchrotron peaked blazars (HBLs): 1ES 0229+200, 1ES 0414+009, PKS 0548-322, 1ES 1101-232, 1H 1219+301, H 1426+428, Mrk 501, 1ES 1959+650, PKS 2005-489, and 1ES
Externí odkaz:
http://arxiv.org/abs/2209.05515
Autor:
Ismail, Said I., Al-Muftah, Wadha, Badji, Radja, Mbarek, Hamdi, Darwish, Dima, Fadl, Tasnim, Yasin, Heba, Ennaifar, Maryem, Abdellatif, Rania, Alkuwari, Fatima, Alvi, Muhammad, Al-Sarraj, Yasser, Saad, Chadi, Althani, Asmaa, Fethnou, Eleni, Qafoud, Fatima, Alkhayat, Eiman, Afifi, Nahla, Tomei, Sara, Liu, Wei, Lorenz, Stephan, Syed, Najeeb, Almabrazi, Hakeem, Vempalli, Fazulur Rehaman, Temanni, Ramzi, Saqri, Tariq Abu, Khatib, Mohammedhusen, Hamza, Mehshad, Zaid, Tariq Abu, El Khouly, Ahmed, Pathare, Tushar, Poolat, Shafeeq, Al-Ali, Rashid, Albagha, Omar, Al-Khodor, Souhaila, Alshafai, Mashael, Badii, Ramin, Chouchane, Lotfi, Estivill, Xavier, Fakhro, Khalid A., Mokrab, Younes, Puthen, Jithesh V., Suhre, Karsten, Tatari, Zohreh, Devadoss Gandhi, Geethanjali, Aliyev, Elbay, Al-Saei, Omayma, Al-Maraghi, Aljazi, Abdi, Mona, Krishnamoorthy, Navaneethakrishnan, Akil, Ammira A., Ben-Omran, Tawfeg
Publikováno v:
In Genetics in Medicine December 2024 26(12)
