activity
19972017
most citedMillisecond radio pulsars with known masses: parameter values and equation of state models

25 citations · 56 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2017★ 18 cited

Two coexisting families of compact stars: observational implications for millisecond pulsars

Sudip Bhattacharyya, Ignazio Bombaci, Domenico Logoteta +1

It is usually thought that a single equation of state (EoS) model "correctly" represents cores of all compact stars. Here we emphasize that two families of compact stars, viz., neu…

astro-ph.HE2017★ 25 cited

Millisecond radio pulsars with known masses: parameter values and equation of state models

Sudip Bhattacharyya, Ignazio Bombaci, Debades Bandyopadhyay +2

The recent fast growth of a population of millisecond pulsars with precisely measured mass provides an excellent opportunity to characterize these compact stars at an unprecedented…

astro-ph2004

Differentially rotating magnetised neutron stars: production of toroidal magnetic fields

A. V. Thampan

We initiate numerical studies of differentially rotating magnetised (proto) neutron stars by studying - through construction from first principles - the coupling between an assumed…

gr-qc2003★ 13 cited

The Hartle-Thorne circular geodesics

M. A. Abramowicz, G. J. E. Almergren, W. Kluzniak +1

The Hartle-Thorne metric is an exact solution of vacuum Einstein field equations that describes the exterior of any slowly and rigidly rotating, stationary and axially symmetric bo…

astro-ph2001

General Relativistic Spectra from Accretion Disks around Rapidly Rotating Neutron Stars

Sudip Bhattacharyya, Dipankar Bhattacharya, Ranjeev Misra +1

We compute spectra from accretion disks around rapidly rotating neutron stars. The full effect of general relativity is considered for the structure calculation of the stars. We ta…

astro-ph1999

Possible signatures for strange stars in stellar X-ray binaries

Bhaskar Datta, Arun V. Thampan, Ignazio Bombaci

Kilohertz quasi-periodic brightness oscillations (kHz QPOs) observed in certain X-ray burst sources may represent Keplerian frequencies in the inner regions of the accretion disk i…