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Results 1-10 of 34 (Search time: 0.007 seconds).
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Issue Date
Title
Author(s)
2006
Deep J -band imaging of high redshift QSO candidates with the Himalayan Chandra Telescope
Goto, T
;
Ojha, D
2009-02
2.5-dimensional solution of the advective accretion disk: a self-similar approach
Ghosh, S
;
Mukhopadhyay, B
2014-08-10
Probing the Active Massive Black Hole Candidate in the Center of NGC 404 with VLBI
Paragi, Z
;
Frey, S
;
Kaaret, P
;
Cseh, D
;
Overzier, R
;
Preethi, K
2014-08-20
X-ray variability and the inner region in active galactic nuclei
Mohan, Prashanth
;
Mangalam, A
2012-06
TeV blazar variability: the firehose instability?
Subramanian, P
;
Shukla, A
;
Becker, P. A
2017-06
Accretion and wind dynamics in tidal disruption events
Mageshwaran, T
;
Mangalam, A
2014-06
Probing the physics of narrow-line regions of Seyfert galaxies, I. The case of NGC 5427
Dopita, M. A
;
Scharwachter, J
;
Shastri, P
;
Kewley, L. J
;
Davies, R
;
Sutherland, R
;
Kharb, P
;
Jose, J
;
Hampton, E
;
Jin, C
;
Banfield, J
;
Basurah, H
;
Fischer, S
2015-03-01
Probing the physics of narrow-line regions in active galaxies. III. accretion and cocoon shocks in the liner NGC 1052
Dopita, M. A
;
Ho, I-Ting
;
Dressel, L. L
;
Sutherland, R
;
Kewley, L
;
Davies, R
;
Hampton, E
;
Shastri, P
;
Kharb, P
;
Jose, Jessy
;
Bhatt, H. C
;
Ramya, S
;
Scharwachter, J
;
Jin, C
;
Banfield, J
;
Zaw, I
;
James, B
;
Juneau, S
;
Srivastava, S
2018-12
Polarization and QPOs from jets in black hole systems
Mangalam, A
2016-12-10
The detection of Diffuse Extended Structure in 3C 273: implications for jet power
Punsly, B
;
Kharb, P
Discover
Author
9
Mangalam, A
6
Mondal, Santanu
4
Kharb, P
4
Nandi, Anuj
4
Stalin, C. S
3
Chakrabarti, S. K
3
Das, Santabrata
3
Mageshwaran, T
3
Sreehari, H
2
Banfield, J
.
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Subject
11
Galaxies: jets
10
Accretion
10
Galaxies: active
6
X-rays: binaries
5
Accretion, accretion discs
4
Accretion discs
4
Accretion, accretion disks
4
Hydrodynamics
4
Shock waves
3
Accretion disks
.
next >
Date issued
15
2020 - 2023
17
2010 - 2019
2
2006 - 2009
Has File(s)
34
true