Zobrazeno 1 - 10
of 14
pro vyhledávání: '"N. D. Vagshette"'
Publikováno v:
Serbian Astronomical Journal, Vol 2021, Iss 202, Pp 17-24 (2021)
We present results based on analysis of the currently available 29.86 ks Chandra data on the Bright Group-Centered Galaxy (BGG) NGC 5846 of G50 group. A pair of X-ray cavities have been detected within a radius ? 1 kpc along the North-East and South-
Publikováno v:
Journal of Astrophysics and Astronomy. 42
We present imaging and photometric studies of the radio galaxy NGC 1316 (Fornax~A) using high spatial resolution near-ultraviolet (NUV) and far-ultraviolet (FUV) imaging telescopes of the first Indian multi-wavelength space observatory {\it AstroSat}
We present results obtained from the analysis of a total of 110 ks Chandra observations of 3C 320 FR II radio galaxy, located at the centre of a cluster of galaxies at a redshift $z=0.342$. A pair of X-ray cavities have been detected at an average di
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7573dd71cbe6d75728f5b10433b0261f
http://arxiv.org/abs/1902.04778
http://arxiv.org/abs/1902.04778
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 466:2054-2066
We present results obtained from a detailed analysis of a deep Chandra observation of the bright FR II radio galaxy 3C~444 in Abell~3847 cluster. A pair of huge X-ray cavities are detected along North and South directions from the centre of 3C 444. X
Publikováno v:
Research in Astronomy and Astrophysics. 13:885-898
We present multi-wavelength imagery of the merger remnant galaxy NGC 1316 with an objective to study the dust content and its association with the other phases of the interstellar medium. Color-index maps as well as extinction maps derived for this g
We present the results obtained from a total of 123 ks X-ray (Chandra) and 8 hrs of 1.4 GHz radio (Giant Metrewave Radio Telescope - GMRT) observations of the cool core cluster ZwCl 2701 (z = 0.214). These observations of ZwCl 2701 showed the presenc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4a6d054dd4614df99562457620c79c9c
http://arxiv.org/abs/1606.04651
http://arxiv.org/abs/1606.04651
Autor:
Y. K. Arora, Varun Bhalerao, Essy Samuel, Santosh V. Vadawale, M. H. Patil, Dipankar Bhattacharya, S. Sinha, P. Priya, K. S. Sarma, S. Sreekumar, N. D. Vagshette, S. Seetha, N. P. S. Mithun, K. H. Navalgund, A. P. K. Kutty, A. R. Rao, R. Pandiyan, K. Subbarao, A. Vibhute, P. Vinod, M. K. Hingar, J. P. Malkar, P. K. Pawar, Rakesh Khanna
Publikováno v:
NASA Astrophysics Data System
The Cadmium Zinc Telluride Imager (CZTI) is a high energy, wide-field imaging instrument on AstroSat. CZT's namesake Cadmium Zinc Telluride detectors cover an energy range from 20 keV to > 200 keV, with 11% energy resolution at 60 keV. The coded aper
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0cfb0072ceb41b69a5a7d5e086656b39
Publikováno v:
New Astronomy. 17:524-532
We present the results based on multiwavelength imaging observations of the prominent dust lane starburst galaxy NGC 1482 aimed to investigate the extinction properties of dust existing in the extreme environment. (B-V) colour-index map derived for t
We present results based on the systematic analysis of high resolution 95 ks Chandra observations of the strong cool core cluster Abell 2390 at the redshift of z= 0.228 that hosts an energetic radio AGN. This analysis has enabled us to investigate fi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9c1f5d6d193990813cb3579b66c814c0
http://arxiv.org/abs/1412.8632
http://arxiv.org/abs/1412.8632
Autor:
Debdutta Paul, A. P. K. Kutty, Tanmoy Chattopadhyay, R. Pandiyan, A. R. Rao, N. P. S. Mithun, Gulab C. Dewangan, S. Seetha, Varun Bhalerao, P. K. Pawar, K. Subbarao, S. Sreekumar, P. Pradeep, N. D. Vagshette, A. Vibhute, P. Vinod, Vikas Chand, Rakesh Khanna, Dipankar Bhattacharya, M. K. Hingar, J. P. Malkar, Rupal Basak, Essy Samuel, Santosh V. Vadawale, K. H. Navalgund, K. S. Sarma, Shabnam Iyyani
Publikováno v:
The Astrophysical Journal. 833:86
AstroSat is a multi-wavelength satellite launched on 2015 September 28. The CZT Imager of AstroSat on its very first day of operation detected a long duration gamma-ray burst (GRB) namely GRB 151006A. Using the off-axis imaging and spectral response