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20202026
most citedGaia18aen: First symbiotic star discovered by Gaia

22 citations · 23 across the 9 of their papers we have counts for

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Showing 2026Show all

6 papers · 1 filter

astro-ph.SR2026

Dynamically driven collapse of a thermally stable accretion disk in a nova-like system

Wentao Li, Jie Lin, Tinggui Wang +8

While standard disk instability theory predicts thermal-steady, outburst-free disks in nova-like variables due to their high mass transfer rates, mass transfer variations are preva…

astro-ph.HE2026

A Systematic Search for Optical Outbursts in IPs Using ASAS-SN

Jake Mendelsohn, Simone Scaringi, Martina Veresvarska +1

Cataclysmic variables can show rapid increases in optical flux. Intermediate polars (IPs), a subset with strong magnetic fields that disrupt the inner accretion disc, have been tho…

astro-ph.SR2026

TESS light curves of two new magnetic cataclysmic variables: an asynchronous polar at the period minimum, and an eclipsing system with a large spin-to-orbit ratio

Colin Littlefield, Krystian Ilkiewicz, Paul A. Mason +2

A recent development in the study of magnetic cataclysmic variable stars (mCVs) has been the identification of asynchronously spinning mCVs with orbital periods <2 h that have sign…

astro-ph.SR2026

A Catalogue of Orbital Periods of Cataclysmic Variables and Candidates from TESS Observations

Meryem K. Dağ, Simone Scaringi, Kieran O'Brien +21

We present a systematic analysis of 2544 cataclysmic variable systems and related candidates observed by the Transiting Exoplanet Survey Satellite (TESS), with the aim of compiling…

astro-ph.SR2026

The Inner and Outer Shock Layers of Bow Shocks in Cataclysmic Variables

Krystian Ilkiewicz, Christian Knigge, Simone Scaringi +3

Bow shocks around cataclysmic variables (CVs) have traditionally been identified with a single bright optical arc. This feature has been interpreted as the bow shock formed by the…

astro-ph.SR2026★ 1 cited

A persistent bow shock in a diskless magnetised accreting white dwarf

Krystian Ilkiewicz, Simone Scaringi, Domitilla de Martino +9

Stellar bow shocks are formed when an outflow interacts with the interstellar medium. In white dwarfs accreting from a binary companion, outflows are associated with either strong…