activity
20082023
most citedA Radio Pulsar/X-ray Binary Link

591 citations · 2k across the 51 of their papers we have counts for

collaborators

53 papers

astro-ph.SR2023

TIC 378898110: A Bright, Short-Period AM CVn Binary in TESS

Matthew J. Green, J. J. Hermes, Brad N. Barlow +22

AM CVn-type systems are ultracompact, helium-accreting binary systems which are evolutionarily linked to the progenitors of thermonuclear supernovae and are expected to be strong G…

astro-ph.SR2023★ 10 cited

An Eclipsing 47 minute Double White Dwarf Binary at 400 pc

James Munday, P. -E. Tremblay, J. J. Hermes +20

We present the discovery of the eclipsing double white dwarf (WD) binary WDJ 022558.21-692025.38 that has an orbital period of 47.19 min. Following identification with the Transiti…

astro-ph.SR2023★ 21 cited

Hot subdwarfs in close binaries observed from space II: Analysis of the light curves

V. Schaffenroth, B. N. Barlow, I. Pelisoli +2

Hot subdwarfs in close binaries with either M dwarf, brown dwarf or white dwarf companions show unique light variations. In hot subdwarf binaries with M dwarf or brown dwarf compan…

astro-ph.SR2023★ 3 cited

V907 Sco Switched to the Eclipsing Mode Again

P. Zasche, D. Vokrouhlický, B. N. Barlow +1

V907 Scorpii is a unique triple system in which the inner binary component has been reported to have switched on and off eclipses several times in modern history. In spite of its p…

astro-ph.SR2022★ 58 cited

Hot subdwarfs in close binaries observed from space I: orbital, atmospheric, and absolute parameters and the nature of their companions

V. Schaffenroth, I. Pelisoli, B. N. Barlow +2

About a third of the hot subdwarfs of spectral type B, which are mostly core-helium burning objects on the extreme horizontal branch, are found in close binaries with cool, low-mas…

astro-ph.SR2022★ 6 cited

Towards a consistent model of the hot quadruple system HD 93206 = QZ Carinæ: II. N-body model

M. Brož, P. Harmanec, P. Zasche +16

HD 93206 is early-type massive stellar system, composed of components resolved by direct imaging (Ab, Ad, B, C, D) as well as a compact sub-system (Aa1, Aa2, Ac1, Ac2). Its geometr…