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Modelling the recurrent nova U Scorpii in quiescence

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arxiv 1305.3424 v1 pith:ANINYXFT submitted 2013-05-15 astro-ph.SR

M. P. Maxwell , M. T. Rushton , S. P. S. Eyres This is my paper · ORCID
classification astro-ph.SR
keywords companionmonthsaccretionbecomeclassconfidenceconstraineddisc
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abstract

VLT and SALT spectroscopy of U Sco were obtained $\sim$18 and $\sim$30 months after the 2010 outburst. From these spectra the accretion disc is shown to take at least 18 months to become fully reformed. The spectral class of the companion is constrained to be F8$^{+5}_{-6}$\,IV-V at the 95% confidence level when the irradiated face of the companion is visible.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs

    astro-ph.HE 2025-05 conditional novelty 5.0 of 10

    The authors claim a common inverse t_rec-mdot relation for thermonuclear runaways on neutron stars and white dwarfs, despite weak correlation in their own compiled data.

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