activity
20002023
most citedThe binary properties of the pulsating subdwarf B eclipsing binary PG 1336-018 (NY Vir)

91 citations · 1.9k across the 76 of their papers we have counts for

collaborators

77 papers

astro-ph.SR2023★ 2 cited

Abundance analysis of a nitrogen-rich extreme-helium hot subdwarf from the SALT survey

L. J. A. Scott., C. S. Jeffery, D. Farren +2

We have performed a detailed spectral analysis of the helium-rich hot subdwarf EC 20187-4939 using data obtained in the SALT survey of helium-rich hot subdwarfs. We have measured i…

astro-ph.SR2023★ 11 cited

Hot white dwarfs and pre-white dwarfs discovered with SALT

C. S. Jeffery, K. Werner, D. Kilkenny +3

The Southern African Large Telescope (SALT) survey of helium-rich hot subdwarfs aims to explore evolutionary pathways amongst groups of highly-evolved stars. The selection criteria…

astro-ph.SR2022★ 2 cited

TESS uncloaks the secondaries in hydrogen-deficient binaries

C. Simon Jeffery

Sgr is the prototype of four known hydrogen-deficient binary (HdB) systems. These are characterised by a hydrogen-deficient A-type primary, variable hydrogen emission li…

astro-ph.SR2022★ 7 cited

Spectroscopic analysis of BPS CS 22940-0009: connecting evolved helium stars

E. J. Snowdon, L. J. A. Scott, C. S. Jeffery +1

BPS CS 22940-0009 is a helium-rich B-star that shares characteristics with both helium-rich B subdwarfs and extreme helium stars. The optical spectrum of BPS CS 22940-0009 has been…

astro-ph.SR2022★ 3 cited

Spectrum synthesis for radially pulsating stars with shocked atmospheres

C. Simon Jeffery

SPEC_PULS describes a suite of computer programs to simulate the emergent spectrum from a radially-pulsating star. It combines a Christy-type non-linear pulsation code with classic…

astro-ph.SR2022★ 18 cited

The OmegaWhite Survey for Short-Period Variable Stars VII: High amplitude, short period blue variables

G. Ramsay, P. A. Woudt, T. Kupfer +11

Blue Large Amplitude Pulsators (BLAPs) are a relatively new class of blue variable stars showing periodic variations in their light curves with periods shorter than a few tens of m…