output
20072022
most citedAsteroids' physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution

85 citations

Showing astro-ph.SRShow all

10 papers · 1 filter

astro-ph.SR2017★ 8 cited

Orbital Period Changes in WZ Sagittae

Joseph Patterson, Geoffrey Stone, Jonathan Kemp +19

We report a long-term (1961-2017) study of the eclipse times in the dwarf nova WZ Sagittae, in an effort to learn its rate of orbital-period change. Some wiggles with a time scale…

astro-ph.SR2017★ 78 cited

Supernovae 2016bdu and 2005gl, and their link with SN 2009ip-like transients: another piece of the puzzle

A. Pastorello, C. S. Kochanek, M. Fraser +52

Supernova (SN) 2016bdu is an unusual transient resembling SN 2009ip. SN 2009ip-like events are characterized by a long-lasting phase of erratic variability which ends with two lumi…

astro-ph.SR2017★ 4 cited

MN Draconis - peculiar, active dwarf nova in the period gap

K. Bakowska, A. Olech, R. Pospieszynski +7

Context: We present results of an extensive world-wide observing campaign of MN Draconis. Aims: MN Draconis is a poorly known active dwarf nova in the period gap and is one of the…

astro-ph.SR2016★ 14 cited

A 16-Year Photometric Campaign on the Eclipsing Novalike Variable DW Ursae Majoris

D. R. S. Boyd, E. de Miguel, J. Patterson +29

We present an analysis of photometric observations of the eclipsing novalike variable DW UMa made by the CBA consortium between 1999 and 2015. Analysis of 372 new and 260 previousl…

astro-ph.SR2015★ 24 cited

Accretion-disc precession in UX Ursae Majoris

E. de Miguel, J. Patterson, D. Cejudo +25

We report the results of a long campaign of time-series photometry on the nova-like variable UX Ursae Majoris during 2015. It spanned 150 nights, with ~1800 hours of coverage on 12…

astro-ph.SR2013★ 27 cited

The helium-rich cataclysmic variable SBSS 1108+574

P. J. Carter, D. Steeghs, E. de Miguel +12

We present time-resolved spectroscopy and photometry of the dwarf nova SBSS 1108+574, obtained during the 2012 outburst. Its quiescent spectrum is unusually rich in helium, showing…