Zobrazeno 1 - 10
of 25
pro vyhledávání: '"Prajapati, Prachi"'
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:
Uppal, Namita, Ganesh, Shashikiran, Joshi, Santosh, Sarkar, Mrinmoy, Prajapati, Prachi, Dileep, Athul
Dust is a ubiquitous component in our Galaxy. It accounts for only $1\%$ mass of the ISM but still is an essential part of the Galaxy. It affects our view of the Galaxy by obscuring the starlight at shorter wavelengths and re-emitting in longer wavel
Externí odkaz:
http://arxiv.org/abs/2311.09617
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:
In Journal of the Academy of Nutrition and Dietetics September 2024 124(9):1206-1213
Autor:
Kasarla, Prashanth Kumar, Patwal, Pitamber Singh, Adalja, Hitesh Kumar L., Mathur, Satya Narain, Sarkar, Deekshya Roy, Singh, Alka, Rai, Archita, Prajapati, Prachi Vinod, Naik, Sachindra, Shah, Amish B., Ganesh, Shashikiran, Baliyan, Kiran S.
Publikováno v:
Proc. SPIE 11447, Ground-based and Airborne Instrumentation for Astronomy VIII, 114476U, 2020
Near-infrared Imager Spectrometer and Polarimeter (NISP) is a camera, an intermediate resolution spectrograph and an imaging polarimeter being developed for upcoming 2.5m telescope of Physical Research Laboratory at Mount Abu, India. NISP is designed
Externí odkaz:
http://arxiv.org/abs/2012.08813
Autor:
Sarkar, Deekshya Roy, Shah, Amish B., Singh, Alka, Patwal, Pitamber Singh, Kasarla, Prashanth Kumar, Rai, Archita, Prajapati, Prachi Vinod, Adalja, Hitesh Kumar L., Mathur, Satya N., Naik, Sachindra, Ganesh, Shashikiran, Baliyan, Kiran S.
Publikováno v:
Proc. SPIE 11447, Ground-based and Airborne Instrumentation for Astronomy VIII, 1144778, 2020
NISP, a multifaceted near-infrared instrument for the upcoming 2.5m IR telescope at MIRO Gurushikhar, Mount Abu, Rajasthan, India is being developed at PRL, Ahmedabad. NISP will have wide (FOV = 10' x 10') field imaging, moderate (R=3000) spectroscop
Externí odkaz:
http://arxiv.org/abs/2012.08805
Autor:
Ganesh, Shashikiran, Rai, Archita, K, Aravind, Singh, Alka, Prajapati, Prachi Vinod, Mishra, Ashish, Kasarla, Prashanth, Sarkar, Deekshya Roy, Patwal, Pitamber Singh, Uppal, Namita, Chandra, Sunil, Mathur, Satyanarain, Shah, Amish B, Baliyan, Kiran S, Joshi, U C
Publikováno v:
Proc. SPIE 11447, Ground-based and Airborne Instrumentation for Astronomy VIII, 114479E, 2020
An Andor 1K $\times$ 1K EMCCD detector has been used to develop an optical imaging polarimeter for use at the Cassegrain focus of 1.2 m telescope of PRL. The optics is derived from an older single-element detector instrument and consists of a rotatin
Externí odkaz:
http://arxiv.org/abs/2012.08768
Autor:
Rai, Archita, Ganesh, Shashikiran, Paul, Sukamal K., Kasarla, Prashanth K., Prajapati, Prachi V., Sarkar, Deekshya R., Singh, Alka, Patwal, Pitambar S., Adalja, Hitesh K L, Mathur, Satya N., Naik, Sachindra, Shah, Amish B., Baliyan, Kiran S.
Publikováno v:
Proc. SPIE 11447, Ground-based and Airborne Instrumentation for Astronomy VIII, 1144765, 2020
As a Near-IR instrument to PRL's upcoming 2.5 m telescope, NISP is designed indigeniously at PRL to serve as a multifaceted instrument. Optical, Mechanical and Electronics subsystems are being designed and developed in-house at PRL. It will consist o
Externí odkaz:
http://arxiv.org/abs/2012.08563
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Prajapati, Prachi, Tej, Anandmayee, del Palacio, Santiago, Benaglia, Paula, CH, Ishwara-Chandra, Vig, Sarita, Mandal, Samir, Ghosh, Swarna Kanti
The supersonic winds produced by massive stars carry a large amount of kinetic power. In numerous scenarios such winds have been proven to produce shocks in which relativistic particles are accelerated emitting non-thermal radiation. Here, we report
Externí odkaz:
http://arxiv.org/abs/1909.12332