Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Bhattacharyya, Dipanweeta"'
Mergers of black holes and other compact objects produce gravitational waves which carry a part of the energy, momentum, and angular momentum of the system. Due to asymmetry in the gravitational wave emission, a recoil kick velocity is imparted to th
Externí odkaz:
http://arxiv.org/abs/2308.05598
Publikováno v:
ApJ 895 130 (2020)
We build an evolution model of the central black hole that depends on the processes of gas accretion, the capture of stars, mergers as well as electromagnetic torque. In case of gas accretion in the presence of cooling sources, the flow is momentum-d
Externí odkaz:
http://arxiv.org/abs/2004.05000
Publikováno v:
Journal of Astrophysics and Astronomy (2018), Vol 39, 4
To investigate the $M_\bullet -\sigma$ relation, we consider realistic elliptical galaxy profiles that are taken to follow a single power law density profile given by $\rho(r) = \rho_{0}(r/ r_{0})^{-\gamma}$ or the Nuker intensity profile. We calcula
Externí odkaz:
http://arxiv.org/abs/1710.05672
To investigate the $M_\bullet -��$ relation, we consider realistic elliptical galaxy profiles that are taken to follow a single power law density profile given by $��(r) = ��_{0}(r/ r_{0})^{-��}$ or the Nuker intensity profile. We cal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e783950a1baca67812bd6511995d2623
Publikováno v:
NASA Astrophysics Data System
To investigate the $M_\bullet -\sigma$ relation, we consider realistic elliptical galaxy profiles that are taken to follow a single power law density profile given by $\rho(r) = \rho_{0}(r/ r_{0})^{-\gamma}$ or the Nuker intensity profile. We calcula
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=arXiv_dedup_::4c366fb7a888b1f3ab90c028fb1c0b52
https://ui.adsabs.harvard.edu/#abs/2017arXiv171005672B
https://ui.adsabs.harvard.edu/#abs/2017arXiv171005672B