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19982025
most citedEnsemble Asteroseismology of Solar-Type Stars with the NASA Kepler Mission

322 citations

Showing 2017Show all

6 papers · 1 filter

astro-ph.GA2017★ 9 cited

Planetary Nebulae with Ultra-Violet Imaging Telescope (UVIT): Far Ultra-violet halo around the Bow Tie nebula (NGC 40)

N. Kameswara Rao, F. Sutaria, J. Murthy +3

Context. NGC 40 is a planetary nebula with diffuse X-ray emission, suggesting an interaction of the high speed wind from WC8 central star (CS) with the nebula. It shows strong Civ…

astro-ph.HE2017★ 21 cited

Modelling type IIP/IIL supernovae interacting with recent episodic mass ejections from their presupernova stars with MESA & SNEC

Sanskriti Das, Alak Ray

We show how dense compact discrete shells of circumstellar gas immediately outside the red supergiants affect the optical light curves of type II-P/II-L SNe taking the example of S…

quant-ph2017★ 1 cited

Rigorous Quantum Limits on Monitoring Free Masses and Harmonic Oscillators

S. M. Roy

There are heuristic arguments proposing that the accuracy of monitoring position of a free mass is limited by the standard quantum limit (SQL):$σ^2 (X(t)) \geq σ^2 (X(0)) +(t^2…

astro-ph.HE2017★ 17 cited

Gravitomagnetism and Pulsar Beam Precession near a Kerr Black Hole

Prashant Kocherlakota, Pankaj S. Joshi, Sudip Bhattacharyya +3

A rotating black hole causes the spin-axis of a nearby pulsar to precess due to geodetic and gravitomagnetic frame-dragging effects. The aim of our theoretical work here is to expl…

hep-ph2017★ 6 cited

A Lower Bound on Inelasticity in Pion-Pion Scattering

André Martin, S. M. Roy

Assuming that the pion-pion scattering amplitude and its absorptive part are analytic inside an ellipse in - plane with foci , and right extremity , ($ε…

astro-ph.SR2017★ 51 cited

Seismic measurement of the locations of the base of convection zone and helium ionization zone for stars in the {\it Kepler} seismic LEGACY sample

Kuldeep Verma, Keyuri Raodeo, H. M. Antia +4

Acoustic glitches are regions inside a star where the sound speed or its derivatives change abruptly. These leave a small characteristic oscillatory signature in the stellar oscill…