I. A.
3 Papers
I. A. is an academic researcher. The author has contributed to research in topics: Blazar & Supermassive black hole. The author has co-authored 3 publications.
Chat about Author
Papers
Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164
A Roy,V. R. Chitnis,Sergio A. Cellone,C. M. Raiteri,Gustavo E. Romero,Paul J. Wiita,Anasua Chatterjee,Jorge Ariel Combi,Mai Liao,Arkadipta Sarkar,Massimo Villata Department of High Energy Physics,T. I. O. F. Research,Homi Bhabha Road,Mumbai-400005,Indian,Aryabhatta Research Institute of Observational Sciences,Manora Peak,Nainital 263001,Key laboratory for Research in Galaxies,Cosmology,Shanghai Observatory,Chinese Academy of Sciences,Shanghai 200030,China.,Complejo Astronomico el Leoncito,San Juan,Argentina,Facultad de Ciencias Astron'omicas y Geof'i sicas,Universidad Nacional de La Plata,La Plata,Buenos Aires,I. Torino,20 viaOsservatorio,I. P. Torinese,Italy.,I. A.,D. Physics,The State University of New Jersey,2000 Pennington Rd.,Ewing,NJ 08628-0718,Usa,Deptamento de Ingenier'ia Mec'anica y Minera,Univ. de Ja'en,Campus Las Lagunillas sn Ed. A3 Ja'en,23071,Spain.,Cas Key Laboratory for Research in Galaxies,D. O. Astronomy,U. O. Science,Technology of China,Hefei,Anhui 230026,School of Astronomy,S. Science,Deutsches Elektronen-Synchrotron,6. Platanenallee,D. Zeuthen,German +58 more
TL;DR: In this paper , a long-term and intraday variability study of optical multi-waveband (U BV RI) data from the blazar AO 0235+164 collected by various telescopes for ∼44 yr (1975-2019).
2
Study of the 12 C + 16 O fusion reaction in carbon burning via the Trojan Horse Method
A. A. Oliva,Aurora Tumino,Neven Soić,Pranav Prajapati,L. Acosta,R. Alba,F. G. Barba,S. Cherubini,Giuseppe D’Agata,D. Dell'Aquila,A. Di Pietro,P. Figuera,D. Galaviz Redondo,Lorenza Di Guardo,Marisa Gulino,F. Hammache,D. Jelavić Malenica,I. A.,Kilic,M. La Cognata,M. La Commara,L. Lamia,M. Lattuada,C. Maiolino,G. Manicò,M. Mazzocco,Matko Milin,Ma Nanru,A. K. Nurmukhanbetova,Deni Nurkić,Sara Palmerini,T. Parascandolo,D. Pierroutsakou,R. G. Pizzone,R. Popočovski,M. Rapisarda,S. Romano,Domenico Santonocito,M. L. Sergi,Shotter,R. Sparta,A. Spiridon,L. Trache,N. Vukman,H. Yamaguchi +44 more
TL;DR: In this paper , the authors show that at temperatures higher than 10 9 K when most of the carbon is depleted and its abundance is lower than 16 O, the 12 C + 16 O reaction can ignite also in the scenario of explosive carbon burning, and the astrophysical energy region of interest ranges from 3 to 7.2 MeV in the center-of-mass frame.
Beta decay along the N=Z line and its relevance in rp-process and X-Ray bursts
TL;DR: In this article , the total absorption spectroscopy (TAS) technique is applied to calculate the B(GT) distribution in the decay of several N =Z, N=Z+2 and their daughters, of particular relevance in rp-process calculations.