Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Shalini Ganguly"'
Autor:
Shalini Ganguly, Yuan Li, Valeria Olivares, Yuanyuan Su, Francoise Combes, Sampadaa Prakash, Stephen Hamer, Pierre Guillard, Trung Ha
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 10 (2023)
The intracluster medium (ICM) in the centers of galaxy clusters is heavily influenced by the “feedback” from supermassive black holes (SMBHs). Feedback can drive turbulence in the ICM and turbulent dissipation can potentially be an important sour
Externí odkaz:
https://doaj.org/article/d9f77229a7da4fbfb3dcc84116edfdf1
Autor:
Rajyasri Ghosh, Shalini Ganguly
Publikováno v:
Journal of Mycopathological research. 60:515-521
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::591b1002f56a276443ac1f4984ae1fc9
https://doi.org/10.57023/jmycr.60.4.2022.515
https://doi.org/10.57023/jmycr.60.4.2022.515
Autor:
Sergei Dyda, Tim Waters, Paola Rodriguez Hidalgo, Margherita Giustini, Jon M. Miller, John C. Raymond, Shalini Ganguly, Timothy R. Kallman, Daniel Proga, Randall Dannen
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
instname
The warm absorbers observed in more than half of all nearby active galactic nuclei (AGN) are tracers of ionized outflows located at parsec scale distances from the central engine. If the smallest inferred ionization parameters correspond to plasma at
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::33d23029bd10d03a52b3752d9fc99ba5
http://hdl.handle.net/20.500.12666/745
http://hdl.handle.net/20.500.12666/745
Autor:
Shalini Ganguly, Shantanu Desai
Publikováno v:
Astroparticle Physics. 94:17-21
Recently Wei et al (arXiv:1612.09425) have found evidence for a transition from positive time lags to negative time lags in the spectral lag data of GRB 160625B. They have fit these observed lags to a sum of two components: an assumed functional form
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0fd889716e5a2f13974b3bb1178b1565
https://doi.org/10.1016/j.astropartphys.2017.07.003
https://doi.org/10.1016/j.astropartphys.2017.07.003
Autor:
Daniel Proga, Shalini Ganguly
A disk wind can cause perturbations that propagate throughout the disk via diffusive processes. On reaching the inner disk, these perturbations can change the disk luminosity, which in turn, can change the wind mass loss rate, $\dot{M}_w$. It has bee
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ea083bd33d913cbb55e50237888f1095
http://arxiv.org/abs/2001.03791
http://arxiv.org/abs/2001.03791
Autor:
Shalini Ganguly, Daniel Proga
Publikováno v:
Astrophysical Journal; 2/10/2020, Vol. 890 Issue 1, p1-1, 1p