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20122022
most citedGaia DR2 Distances and Peculiar Velocities for Galactic Black Hole Transients

120 citations · 317 across the 11 of their papers we have counts for

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Showing astro-ph.HEShow all

9 papers · 1 filter

astro-ph.HE2022★ 29 cited

Astrometric excess noise in Gaia EDR3 and the search for X-ray binaries

P. Gandhi, D. A. H. Buckley, P. A. Charles +6

Astrometric noise (AEN) in excess of parallax and proper motion is a potential signature of orbital wobble of individual components in binary star systems. The combination of X-ray…

astro-ph.HE2020★ 30 cited

Astrometric excess noise in Gaia DR2 and the search for X-ray emitting binaries

Poshak Gandhi, David A. H. Buckley, Phil Charles +4

Astrometric noise in excess of parallax and proper motion could be a signature of orbital wobble of individual components in binary star systems. The combination of X-ray selection…

astro-ph.HE2020★ 27 cited

Estimation of the black hole spin in LMC X-1 using AstroSat

Sneha Prakash Mudambi, A. Rao, S. B. Gudennavar +2

LMC X-1, a persistent, rapidly rotating, extra-galactic, black hole X-ray binary (BHXB) discovered in 1969, has always been observed in its high soft state. Unlike many other BHXBs…

astro-ph.HE2020★ 23 cited

Orbital period dependent spatial scatter of Galactic Black Hole Transients

P. Gandhi, A. Rao, P. A. Charles +4

There remain significant uncertainties in the origin and evolution of black holes in binary systems, in particular regarding their birth sites and the influence of natal kicks. The…

astro-ph.HE2019★ 25 cited

A stochastic propagation model to the energy dependent rapid temporal behaviour of Cygnus X-1 as observed by AstroSat in the hard state

Bari Maqbool, M. Sneha Prakash, R. Misra +8

We report the results from analysis of six observations of Cygnus X-1 by Large Area X-ray Proportional Counters (LAXPC) and Soft X-ray Telescope (SXT) on-board AstroSat, when the s…

astro-ph.HE2019★ 2 cited

Effect of magnetic flux advection on the dynamics of shock in accretion flow around a rotating black hole

Biplob Sarkar, Anjali Rao

We investigate the dynamical behaviour of a magnetized, dissipative, accretion flow around a rapidly rotating black hole. We solve the magnetohydrodynamic equations and calculate t…

astro-ph.HE2018★ 120 cited

Gaia DR2 Distances and Peculiar Velocities for Galactic Black Hole Transients

Poshak Gandhi, Anjali Rao, Michael A. C. Johnson +2

We report on a first census of Galactic black hole X-ray binary (BHXRB) properties with the second data release (DR2) of {\em Gaia}, focusing on dynamically confirmed and strong ca…

astro-ph.HE2018★ 2 cited

Systematic Analysis of Low/Hard State RXTE Spectra of GX 339-4 to Constrain the Geometry of the System

Kalyani Bagri, Ranjeev Misra, Anjali Rao +2

One of the popular models for the low/hard state of Black Hole Binaries is that the standard accretion disk is truncated and the hot inner region produces via Comptonization, the h…

astro-ph.HE2012★ 37 cited

Why is IGR J17091-3624 so faint? Constraints on distance, mass, and spin from `phase-resolved' spectroscopy of the `heartbeat' oscillations

Anjali Rao, S. V. Vadawale

IGR J17091--3624 is a transient X-ray source and is believed to be a Galactic black hole candidate. Recently, it has received a considerable attention due to the detection of pecul…