Zobrazeno 1 - 10
of 61
pro vyhledávání: '"Srivastava, Mudit K."'
The eruption of Nova V2891 Cygni in 2019 offers a rare opportunity to explore the shock-induced processes in novae ejecta. The spectral evolution shows noticeable differences in the evolution of various oxygen emission lines such as O I 7773 {\AA}, O
Externí odkaz:
http://arxiv.org/abs/2407.09634
Autor:
Kumar, Vipin, Rajpurohit, A. S., Srivastava, Mudit K., Fernández-Trincado, José G., Queiroz, A. B. A.
The time scales of variability in active M dwarfs can be related to their various physical parameters. Thus, it is important to understand such variability to decipher the physics of these objects. In this study, we have performed the low resolution
Externí odkaz:
http://arxiv.org/abs/2307.11574
Autor:
Kumar, Vipin, Srivastava, Mudit K., Banerjee, Dipankar P. K., Woodward, C. E., Munari, Ulisse, Evans, Aneurin, Joshi, Vishal, Dallaporta, Sergio, Page, Kim L.
We present multi-epoch optical and near-infrared observations of the highly reddened, \pion{Fe}{ii} class slow nova V2891 Cygni. The observations span 15 months since its discovery. The initial rapid brightening from quiescence, and the presence of a
Externí odkaz:
http://arxiv.org/abs/2112.13425
Autor:
Srivastava, Mudit K., Kumar, Vipin, Dixit, Vaibhav, Patel, Ankita, Jangra, Mohanlal, Rajpurohit, A. S., Mathur, S. N.
Mt. Abu Faint Object Spectrograph and Camera - Pathfinder (MFOSC-P) is an imager-spectrograph developed for the Physical Research Laboratory (PRL) 1.2m telescope at Gurushikhar, Mt. Abu, India. MFOSC-P is based on a focal reducer concept and provides
Externí odkaz:
http://arxiv.org/abs/2104.00314
SU Lyn, a star that ostensibly appears to be an unremarkable late M type giant, has recently been proposed to be a symbiotic star largely based on its hard X-ray properties. The star does not display, in low-resolution optical spectra, the high excit
Externí odkaz:
http://arxiv.org/abs/2009.03104
Autor:
Rajpurohit, A. S., Kumar, Vipin, Srivastava, Mudit K., Allard, F., Homeier, D., Dixit, Vaibhav, Patel, Ankita
Mt. Abu Faint Object Spectrograph and Camera (MFOSC-P) is an in-house developed instrument for Physical Research Laboratory (PRL) 1.2m telescope at Mt. Abu India, commissioned in February 2019. Here we present the first science results derived from t
Externí odkaz:
http://arxiv.org/abs/2001.05683
Autor:
Banerjee, D. P. K., Srivastava, Mudit K., Ashok, N. M., Munari, U., Hambsch, F. -J., Righetti, G. L., Maitan, A.
Near Infrared (NIR) and optical photometry and spectroscopy are presented for the nova V1831 Aquilae, covering the early decline and dust forming phases during the first $\sim$90 days after its discovery. The nova is highly reddened due to interstell
Externí odkaz:
http://arxiv.org/abs/1709.06585
We present near-infrared (NIR) observations of Nova V5668 Sgr, discovered in outburst on 2015 March 15.634 UT, between 2d to 107d after outburst. NIR spectral features are used to classify it as a FeII class of nova. The spectra follow the evolution
Externí odkaz:
http://arxiv.org/abs/1510.04539
We present multi-epoch near-infrared photo-spectroscopic observations of Nova Cephei 2014 and Nova Scorpii 2015, discovered in outburst on 2014 March 8.79 UT and 2015 February 11.84 UT respectively. Nova Cep 2014 shows the conventional NIR characteri
Externí odkaz:
http://arxiv.org/abs/1509.02660
Autor:
Bryant, Julia J., Motohara, Kentaro, Vernet, Joël R. D., Srivastava, Mudit K., Maiti, Arijit, Kumar, Vipin, Mistry, Bhaveshkumar, Patel, Ankita, Dixit, Vaibhav, Lad, Kevikumar
Publikováno v:
Proceedings of SPIE; July 2024, Vol. 13096 Issue: 1 p130961V-130961V-16, 12965156p
