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20212026
most citedGalactic Extinction: How Many Novae Does it Hide and How Does it Affect the Galactic Nova Rate?

14 citations · 19 across the 6 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2026

Three New Likely Spider Millisecond Pulsar Binaries and Optical Kinematic Tracers of Intrabinary Shocks

Jay Strader, Rebecca Kyer, Laura Chomiuk +9

We report the discovery of three candidate spider millisecond pulsars via multi-wavelength follow-up of unassociated Fermi Large Area Telescope gamma-ray sources. All have optical…

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.SR2026

From Light to Sound: Spectroscopic Evolution & Sonification of the flaring Nova V612 Scuti

Pragati Acharya, Elias Aydi, Kirill V. Sokolovsky +17

We present photometric and spectroscopic observations of the 2017 Galactic nova V612 Sct, whose optical evolution was marked by multiple unusually large maxima. The eruption includ…

astro-ph.SR2026

Optical Spectroscopy and Temporal Evolution of the Nova V1405 Cas

Gesesew R. Habtie, Ramkrishna Das, Elias Aydi +1

This paper presents the findings from our study of nova V1405~Cas over the first 1051 days after the outburst. The study includes an analysis of the photometric light curve evoluti…

astro-ph.SR2026

TESS detection of periodic brightness variations during the rise of classical nova PGIR22akgylf

Kirill V. Sokolovsky, Elias Aydi, Konstantin Malanchev +14

Classical novae are transient events powered by thermonuclear burning in a layer of hydrogen-rich material accreted by a white dwarf from its binary companion. Most classical novae…

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.HE2025★ 1 cited

Multidisciplinary Science in the Multimessenger Era

Eric Burns, Christopher L. Fryer, Ivan Agullo +82

Astrophysical observations of the cosmos allow us to probe extreme physics and answer foundational questions on our universe. Modern astronomy is increasingly operating under a hol…

astro-ph.SR2023★ 4 cited

The physical properties of T Pyx as measured by MUSE I. The geometrical distribution of the ejecta and the distance to the remnant

L. Izzo, L. Pasquini, E. Aydi +8

T Pyx is one of the most enigmatic recurrent novae, and it has been proposed as a potential Galactic type-Ia supernova progenitor. Using spatially-resolved data obtained with MUSE,…

astro-ph.GA2021★ 14 cited

Galactic Extinction: How Many Novae Does it Hide and How Does it Affect the Galactic Nova Rate?

A. Kawash, L. Chomiuk, J. A. Rodriguez +11

There is a longstanding discrepancy between the observed Galactic classical nova rate of yr and the predicted rate from Galactic models of --50 yr.…