Zobrazeno 1 - 10
of 477
pro vyhledávání: '"Ishwara P"'
Autor:
Ishwara P, Naod Mekonnen
Publikováno v:
Cogent Business & Management, Vol 11, Iss 1 (2024)
AbstractThis study examines the relationships between the components of ethical decision-making and the factors that contribute to the ethical decision-making of professional accountants. Survey data from 309 professional accountants was analyzed usi
Externí odkaz:
https://doaj.org/article/0db6ed575b1e4126aa4ca7ca3cc32a04
Autor:
Bheemappa Suresha, Anantha Padmanabha, Amith Ramesh, Ishwara Prasanna Shirankallu, Shiva Charan Mysore Ramalingappa
Publikováno v:
Tribology in Industry, Vol 44, Iss 3, Pp 449-460 (2022)
The scrutinized investigation of tribological performance of castor- mahua oil blends was comprehensively studied in comparison to SAE 20W40. Better miscibility and the negligible difference in density is the prime motive for the formulation of casto
Externí odkaz:
https://doaj.org/article/53329834eea64b468687b5d76252eee9
Autor:
Narang, Mayank, Puravankara, Manoj, Vedantham, H. K., Chandra, C. H. Ishwara, De, Ayanabha, Tyagi, Himanshu, Banerjee, Bihan, Nayak, Prasanta K., Surya, Arun, Shridharan, B., Pathak, Vinod C., Tripathi, Mihir
Coherent radio emission with properties similar to planetary auroral signals has been reported from GJ 1151, a quiescent, slow-rotating mid-M star, by the LOFAR Two-metre (120-170 MHz) Sky Survey (LoTSS). The observed {LOFAR} emission is fairly brigh
Externí odkaz:
http://arxiv.org/abs/2409.18507
Autor:
Saha, Anindya, Tej, Anandmayee, del Palacio, Santiago, De Becker, Michaël, Benaglia, Paula, CH, Ishwara Chandra, Prajapati, Prachi
Publikováno v:
Bulletin de la Societe Royale des Sciences de Liege, 2024, Volume 93, No 2, 491-503
In recent years, systems involving massive stars with large wind kinetic power have been considered as promising sites for investigating relativistic particle acceleration in low radio frequencies. With this aim, we observed two Wolf-Rayet systems, W
Externí odkaz:
http://arxiv.org/abs/2406.16480
Autor:
De Becker, Michael, del Palacio, Santiago, Benaglia, Paula, Tej, Anandmayee, Marcote, Benito, Romero, Gustavo Esteban, Bosch-Ramon, Valenti, Ishwara-Chandra, C. H.
Publikováno v:
Bulletin de la Soci\'et\'e Royale des Sciences de Li\`ege, 2024, Volume 93, No 2, 536-543
Galactic cosmic rays (GCRs) constitute a significant part of the energy budget of our Galaxy, and the study of their accelerators is of high importance in modern astrophysics. Their main sources are likely supernova remnants (SNRs). These objects are
Externí odkaz:
http://arxiv.org/abs/2406.14195
Hub-filament systems (HFSs) being the potential sites of formation of star clusters and high mass stars, provide a test bed for the current theories that attempt to explain star formation globally. It is thus important to study a large number of HFSs
Externí odkaz:
http://arxiv.org/abs/2404.07640
Autor:
Narang, Mayank, Manoj, P., Chandra, Ishwara, Banerjee, Bihan, Tyagi, Himanshu, Tamura, Motohide, Henning, Thomas, Mathew, Blesson, Lazio, Joseph, Surya, Arun, Nayak, Prasanta K.
In this work, we present the results from a study using the Giant Meterwave Radio Telescope (GMRT) to search for radio {emission} from planets around three evolved stars namely $\alpha$~Tau, $\beta$~UMi, and $\beta$~Gem. Both $\alpha$~Tau and $\beta$
Externí odkaz:
http://arxiv.org/abs/2402.11182
Autor:
Verma, Khushboo, Moore, Marina, Wottrich, Stephanie, López, Karla Robles, Aggarwal, Nishant, Bhatt, Zeel, Singh, Aagamjit, Unroe, Bradford, Basheer, Salah, Sachdeva, Nitish, Arora, Prinka, Kaur, Harmanjeet, Kaur, Tanupreet, Hood, Tevon, Marquez, Anahi, Varshney, Tushar, Deng, Nanfu, Ramani, Azaan, Ishwara, Pawanraj, Saeed, Maimoona, Peña, Tatiana López Velarde, Barksdale, Bryan, Guha, Sushovan, Kumar, Satwant
In response to the pressing need for advanced clinical problem-solving tools in healthcare, we introduce BooksMed, a novel framework based on a Large Language Model (LLM). BooksMed uniquely emulates human cognitive processes to deliver evidence-based
Externí odkaz:
http://arxiv.org/abs/2310.11266
Autor:
Saha, Anindya, Tej, Anandmayee, del Palacio, Santiago, De Becker, Michaël, Benaglia, Paula, CH, Ishwara Chandra, Prajapati, Prachi
Large wind kinetic power of Wolf-Rayet (WR) stars make them ideal targets in low radio frequencies to search for non-thermal emission due to relativistic particle acceleration. In this paper, we present observations of two WR stars, WR 114 and WR 142
Externí odkaz:
http://arxiv.org/abs/2309.04736
Publikováno v:
2023
We measure the specific star formation rates of \textit{K}-band selected galaxies from the ELAIS-N1 by stacking GMRT data at 610 MHz. We identify a sample of SFGs, spanning $\rm{0.1\leq\,\textit{z}\,\leq\,1.5}$ and $\rm{10^{8.5}<\,{\textit{M}_{\star}
Externí odkaz:
http://arxiv.org/abs/2307.04152