activity
20002025
most citedAsteroseismic measurement of surface-to-core rotation in a main sequence A star, KIC 11145123

238 citations · 1.9k across the 37 of their papers we have counts for

collaborators

39 papers

astro-ph.SR2025★ 6 cited

Asteroseismic detection of a predominantly toroidal magnetic field in the deep interior of the main-sequence F star KIC 9244992

Masao Takata, Simon J. Murphy, Donald W. Kurtz +2

An asteroseismic analysis has revealed a magnetic field in the deep interior of a slowly-rotating main-sequence F star KIC9244992, which was observed by the Kepler spacecraft for f…

astro-ph.SR2025

The orbital parameters of the binary BLAP HD133729 : advantages of the frequency modulation method

Hiromoto Shibahashi, Donald W. Kurtz, Simon J. Murphy

We derive all the orbital parameters of the blue large-amplitude pulsator (BLAP) in the binary system HD133729 by exploiting the frequency modulation (FM) method, which is based on…

astro-ph.SR2020★ 41 cited

On the first Sct--roAp hybrid pulsator and the stability of p and g modes in chemically peculiar A/F stars

Simon J. Murphy, Hideyuki Saio, Masahide Takada-Hidai +4

Strong magnetic fields in chemically peculiar A-type (Ap) stars typically suppress low-overtone pressure modes (p modes) but allow high-overtone p modes to be driven. KIC 11296437…

astro-ph.SR2020★ 8 cited

Pulsation in the white dwarf HE 1017-1352: confirmation of the class of hot DAV stars

Alejandra D. Romero, L. Antunes Amaral, S. O. Kepler +3

We report the detection of periodic variations on the T_eff ~32 000 K DA white dwarf star HE 1017-1352. We obtained time series photometry using the 4.1 m SOAR telescope on three s…

astro-ph.SR2020

Search for quiet stellar-mass black holes by asteroseismology from space

Hiromoto Shibahashi, Simon J. Murphy

Stars with an initial mass more than ~25 Msun are thought to ultimately become black holes. Then stellar-mass black holes should be ubiquitous but fewer than 20 have been found in…

astro-ph.SR2019

Asteroseismology as a new window to statistics of binaries

Hiromoto Shibahashi, Simon J. Murphy

More than 340 non-eclipsing binaries of A-F stars as primaries at intermediate periods (100-1000 d) were newly found by uninterrupted photometry with ultra high-precision taken ove…