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20202025
most citedSpectroscopic and photometric analysis of symbiotic candidates -- I. Ten candidates on classical symbiotic stars

19 citations · 33 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2025

HD 5501: A Rapidly Evolving Interacting Eclipsing Binary with a Variable Light Curve and H Emission

Richard O. Gray, Christopher. J. Corbally, Sean Curry +19

HD~5501, a hitherto little studied eclipsing binary with an early A-type primary, has been caught in a short-lived, astrophysically interesting phase of its binary evolution. Recen…

astro-ph.SR2023★ 1 cited

TU Tau B: The Peculiar 'Eclipse' of a possible proto-Barium Giant

Richard O. Gray, Christopher J. Corbally, Michael M. Briley +26

TU Tau (= HD 38218 = HIP 27135) is a binary system consisting of a C-N carbon star primary and an A-type secondary. We report on new photometry and spectroscopy which tracked the r…

astro-ph.SR2023

Comprehensive analysis of a symbiotic candidate V503 Her

J. Merc, R. Gális, M. Wolf +10

V503 Her was previously proposed as an eclipsing symbiotic candidate based on photometric behavior and spectroscopic appearance indicating the composite optical spectrum. To invest…

astro-ph.HE2022

V392 Persei: a γ-ray bright nova eruption from a known dwarf nova

F. J. Murphy-Glaysher, M. J. Darnley, É. J. Harvey +57

V392 Persei is a known dwarf nova (DN) that underwent a classical nova eruption in 2018. Here we report ground-based optical, Swift UV and X-ray, and Fermi-LAT γ-ray observations f…

astro-ph.SR2021★ 19 cited

Spectroscopic and photometric analysis of symbiotic candidates -- I. Ten candidates on classical symbiotic stars

J. Merc, R. Gális, M. Wolf +10

Symbiotic stars belong to a group of interacting binaries that display a wide variety of phenomena, including prominent outbursts connected with mass transfer, as well as stellar w…

astro-ph.SR2020★ 13 cited

The path to Z And-type outbursts: The case of V426 Sagittae (HBHA 1704-05)

A. Skopal, S. Yu. Shugarov, U. Munari +16

The star V426 Sge (HBHA~1704-05), originally classified as an emission-line object and a semi-regular variable, brightened at the beginning of August 2018, showing signatures of a…