activity
20032026
most citedKIC 4544587: an Eccentric, Short Period Binary System with delta Sct Pulsations and Tidally Excited Modes

157 citations · 319 across the 35 of their papers we have counts for

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Showing 2024Show all

8 papers · 1 filter

astro-ph.SR2024

Rediscussion of eclipsing binaries. Paper XXII. The B-type system MU Cassiopeiae

John Southworth

MU Cas is a detached eclipsing binary containing two B5 V stars in an orbit of period 9.653 d and eccentricity 0.192, which has been observed in seven sectors using the Transiting…

astro-ph.SR2024

Rediscussion of eclipsing binaries. Paper XXI. The totally-eclipsing B-type system IQ Persei

John Southworth

IQ Per is a totally-eclipsing binary system containing a B8 V star and an A6 V star in an orbit of period 1.744 d with eccentricity and apsidal motion. We use new light curves from…

astro-ph.SR2024

Rediscussion of eclipsing binaries. Paper XX. HO Tel checkout

John Southworth

We present a detailed analysis of the detached eclipsing binary system HO Telescopii, which contains two A-type stars in a circular orbit of period 1.613 d. We use light curves fro…

astro-ph.SR2024

Characterization of the Scuti eclipsing binary KIC 4851217 and its tertiary companion as well as detection of tidally tilted pulsations

Z. Jennings, J. Southworth, S. A. Rappaport +3

Stellar theory enables us to understand the properties of stars at different stages of their evolution, and contributes to other fields of astrophysics such as galactic and exoplan…

astro-ph.SR2024

Rediscussion of eclipsing binaries. Paper XIX. The long-period solar-type system V454 Aurigae

John Southworth

V454 Aur is an eclipsing binary system containing two solar-type stars on an orbit of relatively long period (P = 27.02 d) and large eccentricity (e = 0.381). Eclipses were detecte…

astro-ph.SR2024

Rediscussion of eclipsing binaries. Paper XVIII. The F-type system OO Pegasi

John Southworth

OO Peg is a detached eclipsing binary system containing two late-A-type stars in a circular orbit with a period of 2.985 d. Using published spectroscopic results and a light curve…