Zobrazeno 1 - 10
of 65
pro vyhledávání: '"Kamath, U. S."'
Autor:
Nayak, Prasanta K., Narang, Mayank, Manoj, P., Ojha, D. K., Mathew, Blesson, Baug, T., Chandra, S., Vig, S., Maheswar, G., Kamath, U. S.
The paper demonstrates the spectroscopic and photometric capabilities of the Ultra-Violet Imaging Telescope (UVIT) to study T-Tauri stars (TTSs). We present the first UVIT/Far-UV spectrum of a TTS, TW Hya. Based on C IV line luminosity, we estimated
Externí odkaz:
http://arxiv.org/abs/2403.19478
Autor:
Nayana, A. J., Anupama, G. C., Roy, Nirupam, Banerjee, Dipankar P. K., Singh, Kulinder Pal, S., Sonith L., Kamath, U. S.
We present low-frequency radio observations of the Galactic symbiotic recurrent nova RS Ophiuchi during its 2021 outburst. The observations were carried out with the upgraded Giant Metrewave Radio Telescope (uGMRT) spanning a frequency range of 0.15$
Externí odkaz:
http://arxiv.org/abs/2401.05643
Autor:
Bhargava, Yash, Dewangan, Gulab Chand, Anupama, G. C., Kamath, U. S., Sonith, L. S., Singh, Kulinder Pal, Drake, J. J., Beardmore, A., Luna, G. J. M., Orio, M., Page, K. L.
Nova Her 2021 or V1674 Her was one of the fastest novae to be observed so far. We report here the results from our timing and spectral studies of the source observed at multiple epochs with AstroSat. We report the detection of a periodicity in the so
Externí odkaz:
http://arxiv.org/abs/2312.10291
Publikováno v:
A&A 653, A142 (2021)
The presence of three more Herbig Ae/Be (HAeBe) stars in the Cepheus Flare within a 1.5$^{\circ}$ radius centered on HD 200775 suggests that star formation is prevalent in a wider region of the LDN 1147/1158, LDN 1172/1174, and LDN 1177 clouds. A num
Externí odkaz:
http://arxiv.org/abs/2104.12061
Using our previously reported observations, we derive some physical parameters of the moderately fast nova V2676 Ophiuchi 2012 # 1. The best-fit CLOUDY model of the nebular spectrum obtained on 2015 May 8 shows a hot white dwarf source with Tbb = 1.0
Externí odkaz:
http://arxiv.org/abs/1803.09503
Autor:
Mondal, Anindita, Anupama, G. C., Kamath, U. S., Das, Ramkrishna, Selvakumar, G., Mondal, Soumen
Optical spectra of the 2006 outburst of RS Ophiuchi beginning one day after discovery to over a year after the outburst are presented here. The spectral evolution is found to be similar to that in previous outbursts. The early phase spectra are domin
Externí odkaz:
http://arxiv.org/abs/1711.07643
Stars and planetary systems are formed out of molecular clouds in the interstellar medium. Although the sequence of steps involved in star formation are generally known, a comprehensive theory which describes the details of the processes that drive f
Externí odkaz:
http://arxiv.org/abs/1610.08185
Akademický článek
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Autor:
Skidmore, Warren, Dell'Antonio, Ian, Fukugawa, Misato, Goswami, Aruna, Hao, Lei, Jewitt, David, Laughlin, Greg, Steidel, Charles, Hickson, Paul, Simard, Luc, Schöck, Matthias, Treu, Tommaso, Cohen, Judith, Anupama, G. C., Dickinson, Mark, Harrison, Fiona, Kodama, Tadayuki, Lu, Jessica R., Macintosh, Bruce, Malkan, Matt, Mao, Shude, Narita, Norio, Sekiguchi, Tomohiko, Subramaniam, Annapurni, Tanaka, Masaomi, Tian, Feng, A'Hearn, Michael, Akiyama, Masayuki, Ali, Babar, Aoki, Wako, Bagchi, Manjari, Barth, Aaron, Bhalerao, Varun, Bradac, Marusa, Bullock, James, Burgasser, Adam J., Chapman, Scott, Chary, Ranga-Ram, Chiba, Masashi, Cooper, Michael, Cooray, Asantha, Crossfield, Ian, Currie, Thayne, Das, Mousumi, Dewangan, G. C., de Grijs, Richard, Do, Tuan, Dong, Subo, Evslin, Jarah, Fang, Taotao, Fang, Xuan, Fassnacht, Christopher, Fletcher, Leigh, Gaidos, Eric, Gal, Roy, Ghez, Andrea, Giavalisco, Mauro, Grady, Carol A., Greathouse, Thomas, Gogoi, Rupjyoti, Guhathakurta, Puragra, Ho, Luis, Hasan, Priya, Herczeg, Gregory J., Honda, Mitsuhiko, Imanishi, Masa, Inami, Hanae, Iye, Masanori, Kalirai, Jason, Kamath, U. S., Kane, Stephen, Kashikawa, Nobunari, Kasliwal, Mansi, Kasliwal, Vishal, Kirby, Evan, Konopacky, Quinn M., Lepine, Sebastien, Li, Di, Li, Jianyang, Liu, Junjun, Liu, Michael C., Lopez-Rodriguez, Enrigue, Lotz, Jennifer, Lubin, Philip, Macri, Lucas, Maeda, Keiichi, Marchis, Franck, Marois, Christian, Marscher, Alan, Martin, Crystal, Matsuo, Taro, Max, Claire, McConnachie, Alan, McGough, Stacy, Melis, Carl, Meyer, Leo, Mumma, Michael, Muto, Takayuki, Nagao, Tohru, Najita, Joan R., Navarro, Julio, Pierce, Michael, Prochaska, Jason X., Oguri, Masamune, Ojha, Devendra K., Okamoto, Yoshiko K., Orton, Glenn, Otarola, Angel, Ouchi, Masami, Packham, Chris, Padgett, Deborah L., Pandey, Shashi Bhushan, Pilachowsky, Catherine, Pontoppidan, Klaus M., Primack, Joel, Puthiyaveettil, Shalima, Ramirez-Ruiz, Enrico, Reddy, Naveen, Rich, Michael, Richter, Matthew J., Schombert, James, Sen, Anjan Ananda, Shi, Jianrong, Sheth, Kartik, Srianand, R., Tan, Jonathan C., Tanaka, Masayuki, Tanner, Angelle, Tominaga, Nozomu, Tytler, David, U, Vivian, Wang, Lingzhi, Wang, Xiaofeng, Wang, Yiping, Wilson, Gillian, Wright, Shelley, Wu, Chao, Wu, Xufeng, Xu, Renxin, Yamada, Toru, Yang, Bin, Zhao, Gongbo, Zhao, Hongsheng
The TMT Detailed Science Case describes the transformational science that the Thirty Meter Telescope will enable. Planned to begin science operations in 2024, TMT will open up opportunities for revolutionary discoveries in essentially every field of
Externí odkaz:
http://arxiv.org/abs/1505.01195
Akademický článek
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