Zobrazeno 1 - 10
of 1 836
pro vyhledávání: '"T. R. Seshadri"'
Autor:
Rangaswami, S.
Publikováno v:
Current Science, 1975 Nov . 44(22), 801-802.
Externí odkaz:
https://www.jstor.org/stable/24081901
Publikováno v:
Current Science, 1960 May 01. 29(5), 170-170.
Externí odkaz:
https://www.jstor.org/stable/24214488
Autor:
N. R. Krishnaswamy
Publikováno v:
Resonance. 9:3-5
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f7b9ab04d26b5df7f5f3f76fe0eb95b6
https://doi.org/10.1007/bf02834954
https://doi.org/10.1007/bf02834954
Publikováno v:
Current Science, 1947 Aug 01. 16(8), 262-262.
Externí odkaz:
https://www.jstor.org/stable/24209812
Autor:
Lakshmanan Sriramkumar, T R Seshadri
This book comprises expository articles on different aspects of gravitation and cosmology that are aimed at graduate students. The topics discussed are of contemporary interest assuming only an elementary introduction to gravitation and cosmology. Th
Autor:
S. Suresh Babu, Manish Naja, Umesh Chandra Dumka, Hema Joshi, Mukunda M. Gogoi, T. R. Seshadri, Priyanka Srivastava
Publikováno v:
Asia-Pacific Journal of Atmospheric Sciences. 58:83-96
Accurate estimation of black carbon (BC) from the widely used optical attenuation technique is important for the reliable assessment of their climatic impact. The optical instruments use Mass Absorption Cross-section (MAC) for converting light attenu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::06e37b790a1a9c39a9fe678dea8a9dff
https://doi.org/10.1007/s13143-021-00241-6
https://doi.org/10.1007/s13143-021-00241-6
Implications of baryon–dark matter interaction on IGM temperature and tSZ effect with magnetic field
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 500:643-654
We show that the combined effect of cosmic magnetic field and a possible non-standard interaction between baryons and dark matter has interesting consequences on the thermal Sunyaev$-$Zel${'}$dovich (tSZ) effect depending on the temperature and the i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::614284c69dd0a9978c4a988ab9cce0f7
https://doi.org/10.1093/mnras/staa3281
https://doi.org/10.1093/mnras/staa3281
Astrophysical magnetic fields decay primarily via two processes namely, ambipolar diffusion and turbulence. Constraints on the strength and the spectral index of non-helical magnetic fields have been derived earlier in the literature through the effe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d915537622f017fd78a687efa1859d25
Magnetic fields have been observed in galaxy clusters with strengths of the order of $\sim \mu$G. The non-thermal pressure exerted by magnetic fields also contributes to the total pressure in galaxy clusters and can in turn affect the estimates of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1b3116a9a8a7116964b1799060b7fa31
http://arxiv.org/abs/1909.07847
http://arxiv.org/abs/1909.07847