activity
19982026
most citedEffects of Gravity on the Structure of Postshock Accretion Flows in Magnetic Cataclysmic Variables

122 citations · 3.4k across the 145 of their papers we have counts for

collaborators

146 papers

astro-ph.SR2026

Magnetically guided accretion and extremely slow rotation in a metal-enriched white dwarf

S. Bagnulo, M. A. Stroet, C. P. Folsom +3

White dwarfs that show atmospheric metal enrichment offer a direct window into the bulk composition of exoplanetary material and provide some of the most direct constraints on the…

astro-ph.HE2023

Constraining white dwarf mass and magnetic field strength of a new intermediate polar through X-ray observations

Benjamin Vermette, Ciro Salcedo, Kaya Mori +9

We report a broad-band analysis of a Galactic X-ray source, CXOGBS J174517.0-321356 (J1745), with a 614-second periodicity. Chandra discovered the source in the direction of the Ga…

astro-ph.HE2023★ 13 cited

GRB 201015A and the nature of low-luminosity soft gamma-ray bursts

M. Patel, B. P. Gompertz, P. T. O'Brien +20

GRB 201015A is a peculiarly low luminosity, spectrally soft gamma-ray burst (GRB), with s (time interval of detection of 90\% of photons from the GRB), a…

astro-ph.SR2023★ 8 cited

NGTS clusters survey V: Rotation in the Orion Star-forming Complex

Gareth D. Smith, Edward Gillen, Simon T. Hodgkin +16

We present a study of rotation across 30 square degrees of the Orion Star-forming Complex, following a 200 d photometric monitoring campaign by the Next Generation Transit Su…

astro-ph.SR2023★ 2 cited

NGTS clusters survey IV. Search for Dipper stars in the Orion Nebular Cluster

Tyler Moulton, Simon T Hodgkin, Gareth D Smith +13

The dipper is a novel class of young stellar object associated with large drops in flux on the order of 10 to 50 per cent lasting for hours to days. Too significant to arise from i…

astro-ph.SR2023★ 15 cited

LISA Galactic binaries with astrometry from Gaia DR3

Thomas Kupfer, Valeriya Korol, Tyson B. Littenberg +11

Galactic compact binaries with orbital periods shorter than a few hours emit detectable gravitational waves at low frequencies. Their gravitational wave signals can be detected wit…