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19962023
most citedThe eROSITA X-ray telescope on SRG

884 citations · 6.2k across the 117 of their papers we have counts for

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astro-ph.SR2019★ 43 cited

Comprehensive models of novae at metallicity and

Hai-Liang Chen, T. E. Woods, L. R. Yungelson +3

Novae are the observational manifestations of thermonuclear runaways on the surface of accreting white dwarfs (WDs). Although novae are an ubiquitous phenomenon, their properties a…

astro-ph.SR2018

Populations of accreting white dwarfs

Hai-Liang Chen, Tyrone E. Woods, Lev Yungelson +2

Using a hybrid binary population synthesis approach, we modelled the formation and evolution of populations of accreting WDs for differing star formation histories. We found that t…

astro-ph.SR2018★ 52 cited

Variability of Red Supergiants in M31 from the Palomar Transient Factory

Monika D. Soraisam, Lars Bildsten, Maria R. Drout +9

Most massive stars end their lives as Red Supergiants (RSGs), a short-lived evolution phase when they are known to pulsate with varying amplitudes. The RSG period-luminosity (PL) r…

astro-ph.SR2017★ 32 cited

No hot and luminous progenitor for Tycho's supernova

T. E. Woods, P. Ghavamian, C. Badenes +1

Type Ia supernovae have proven vital to our understanding of cosmology, both as standard candles and for their role in galactic chemical evolution; however, their origin remains un…

astro-ph.SR2016★ 28 cited

Modelling nova populations in galaxies

Hai-Liang Chen, T. E. Woods, L. R. Yungelson +2

Theoretical modelling of the evolution of classical and recurrent novae plays an important role in studies of binary evolution, nucleosynthesis and accretion physics. However, from…

astro-ph.SR2015★ 22 cited

Population of post-nova supersoft X-ray sources

Monika D. Soraisam, Marat Gilfanov, William M. Wolf +1

Novae undergo a supersoft X-ray phase of varying duration after the optical outburst. Such transient post-nova supersoft X-ray sources (SSSs) are the majority of the observed SSSs…