activity
20032026
most citedTwo Types of X-ray Spectra in Cataclysmic Variables

138 citations · 232 across the 12 of their papers we have counts for

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7 papers · 1 filter

astro-ph.HE2026

The First Multi-Messenger Nova: External Shocks, TeV Photons, and Neutrinos in the Next Eruption of T CrB

E. Aydi, P. Craig, K. V. Sokolovsky +10

T Coronae Borealis is the most compelling anticipated Galactic recurrent nova and one of the best opportunities to test whether nova eruptions can become genuine multi-messenger tr…

astro-ph.HE2026

Shocks in the Symbiotic Recurrent Nova V3890 Sgr: VLBI Radio Imaging and Fermi GeV Gamma-Rays

Isabella Molina, Peter Craig, Rebecca Diesing +14

We present very long baseline interferometric (VLBI) radio imaging and Fermi/LAT GeV -ray observations of the 2019 eruption of the symbiotic recurrent nova V3890 Sgr.The VLBI im…

astro-ph.HE2026

Evolution of the recent high-accretion state of the recurrent nova T CrB: HST, Swift, NuSTAR, and XMM-Newton observations

G. J. M. Luna, N. P. M. Kuin, K. Mukai +3

As the recurrent nova T Coronae Borealis (T CrB) approaches its next predicted thermonuclear eruption, it is currently exhibiting a "super-active state" (SAS) characterized by enha…

astro-ph.HE2025

Fermi-LAT detections of novae V1723 Sco and V6598 Sgr

P. Fauverge, P. Jean, K. Sokolovsky +8

Context. Numerous classical novae have been observed to emit γ-rays (E > 100 MeV) detected by the Fermi-LAT. The prevailing hypothesis attributes this emission to the interaction o…

astro-ph.HE2025★ 3 cited

What determines the -ray luminosities of classical novae?

Peter Craig, Elias Aydi, Laura Chomiuk +25

Classical novae in the Milky Way have now been well-established as high-energy GeV -ray sources. In novae with main-sequence companions, this emission is believed to result from…

astro-ph.HE2023

X-rays from RS Ophiuchi's 2021 eruption: shocks in and out of ionization equilibrium

Nazma Islam, Koji Mukai, Jennifer L. Sokoloski

The recurrent nova RS Ophiuchi (RS Oph) underwent its most recent eruption on 8 August 2021 and became the first nova to produce both detectable GeV and TeV emission. We used exten…