activity
20202026
most citedFar UV and Optical Emissions from Three Very Large Supernova Remnants Located at Unusually High Galactic Latitudes

30 citations · 69 across the 9 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2026

Optical Discovery of New and Candidate Galactic Supernova Remnants Plus Optical Imaging of the Monogem Supernova Remnant

Robert A. Fesen, Marcel Drechsler, Bray Falls +16

We report the discovery of new and candidate Galactic supernova remnants made through over 2000 hours of H and [O III] imaging using amateur class instrumentation. These nebulae…

astro-ph.HE2025

The Ejecta Nebula Around the Wolf-Rayet Star WR 71

Robert A. Fesen, Manuel C. Peitsch, Martin R. Pugh +2

We present deep H and [O III] images of the ejecta rich nebulosity associated with the suspected runaway and binary Wolf-Rayet star WR~71 (HD 143414). In H emission, the nebu…

astro-ph.GA2025

SDSO1 is a Shocked Ghost Planetary Nebula in Front of M 31

Patrick Ogle, Mark Petersen, R. Michael Rich +12

We present new, deep narrowband imagery and discuss the nature of SDSO 1, the large [O III]-emitting nebula centered 1.5 degrees SE of M 31. We find strong evidence to support the…

astro-ph.HE2024

Discovery of a [O III] Emission Shell Around the X-ray Binary CI Cam

Robert A. Fesen, Marcel Drechsler, Nicolas Martino +1

We report the serendipitous discovery of a emission shell brightest in [O III] centered on the X-ray binary B[e] star, CI Cameleopardalis (CI Cam). This shell, dete…

astro-ph.HE2024★ 3 cited

Deep Optical Emission-Line Images of Nine Known and Three New Galactic Supernova Remnants

Robert A. Fesen, Marcel Drechsler, Xavier Strottner +14

Deep optical emission-line images are presented for nine known plus three new Galactic supernova remnants (SNRs), all but one having at least one angular dimension greater than one…

astro-ph.SR2023★ 3 cited

Extended far-UV emission surrounding asymptotic giant branch stars as seen by GALEX

V. Răstău, M. Mečina, F. Kerschbaum +5

Aims. Our goal is to study the long-term mass-loss rate characteristics of asymptotic giant branch (AGB) stars through wind-wind and wind-interstellar medium interaction. Methods.…

astro-ph.GA2023

The Spatial and Emission Properties of the Large [O III] Emission Nebula Near M31

Robert A. Fesen, Stefan Kimeswenger, J. Michael Shull +8

Drechsler et al. (2023) reported the unexpected discovery of a 1.5 degree long [O III] emission nebula 1.2 degrees southeast of the M31 nucleus. Here we present additional images o…

astro-ph.SR2021★ 9 cited

YY Hya and its interstellar environment

Stefan Kimeswenger, John R. Thorstensen, Robert A. Fesen +7

During a search for previously unknown Galactic emission nebulae, we discovered a faint 36' diameter Halpha emission nebula centered around the periodic variable YY Hya. Although t…

astro-ph.HE2021★ 30 cited

Far UV and Optical Emissions from Three Very Large Supernova Remnants Located at Unusually High Galactic Latitudes

Robert A. Fesen, Marcel Drechsler, Kathryn E. Weil +9

Galactic supernova remnants (SNRs) with angular dimensions greater than a few degrees are relatively rare, as are remnants located more than ten degrees off the Galactic plane. Her…

astro-ph.HE2020★ 24 cited

G107.0+9.0: A New Large Optically Bright, Radio and X-Ray Faint Galactic Supernova Remnant in Cepheus

Robert A. Fesen, Kathryn E. Weil, John C. Raymond +7

Wide-field H-alpha images of the Galactic plane have revealed a new supernova remnant (SNR) nearly three degrees in diameter centred at l = 107.0, b = +9.0. Deep and higher resolut…