7–12 Jul 2024
Aurum, the ‘Gabriele d’Annunzio’ University and ICRANet
Europe/Rome timezone

Shocked advective flows around black holes and associated observational signatures

11 Jul 2024, 18:00
20m
Aula 35 (‘Gabriele d’Annunzio’ University)

Aula 35

‘Gabriele d’Annunzio’ University

Viale Pindaro, 42, Pescara
Talk in a parallel session Spectral and temporal properties of accretion flows and jets around compact objects and the theoretical models Spectral and temporal properties of accretion flows and jets around compact objects and the theoretical models

Speaker

Chandra Bahadur Singh

Description

Low angular momentum flows around black holes are likely to form standing shocks during the accretion processes. The shocks possibly encounter instabilities leading to various observational signatures associated with inflows and outflows. In our work, we address a range of issues like flaring in under-luminous Sgr A* with supermassive black hole and outflow properties in super-accretors like SS 433 and ultraluminous X-ray sources with stellar-mass black holes.

References:

  1. T. Okuda , C.B. Singh, R. Aktar, 2023, MNRAS, 522, 1814.

  2. T. Okuda , C.B. Singh C.B., R. Aktar, 2022, MNRAS, 514, 5074.

  3. C.B. Singh, T. Okuda, R. Aktar, 2021, RAA, 21, 134.

  4. T. Okuda, C.B. Singh, 2021, MNRAS, 503, 586.

Primary authors

Chandra Bahadur Singh Prof. Toru Okuda (Hokkaido University of Education)

Co-author

Dr Ramiz Aktar (National Tsing Hua University)

Presentation materials

Proceedings

Paper