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20172026
most citedEarly Spectroscopy and Dense Circumstellar Medium Interaction in SN 2023ixf

90 citations · 781 across the 67 of their papers we have counts for

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Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2026

The Eye of Sauron in SN 2025ngs: a Short-plateau Cousin of SN 1998S with Evidence for a Ring-like Circumstellar Medium

Conor L. Ransome, David J. Sand, K. Azalee Bostroem +35

Interacting supernovae probe the twilight years of massive stars, exhibiting signatures of interaction between the supernova ejecta and surrounding material expelled from the proge…

astro-ph.SR2023★ 83 cited

A Luminous Red Supergiant and Dusty Long-period Variable Progenitor for SN 2023ixf

Jacob E. Jencson, Jeniveve Pearson, Emma R. Beasor +23

We analyze pre-explosion near- and mid-infrared (IR) imaging of the site of SN 2023ixf in the nearby spiral galaxy M101 and characterize the candidate progenitor star. The star dis…

astro-ph.SR2023★ 2 cited

A Multi-Year Photopolarimetric Study of the Semi-Regular Variable V CVn and Identification of Analogue Sources

Hilding Neilson, Nicolaus Steenken, John Simpson +4

The semi-regular variable star V Canum Venaticorum (V CVn) is well-known for its unusual linear polarization position angle (PA). Decades of observing V CVn reveal a nearly constan…

astro-ph.SR2023★ 2 cited

Shock shaping? Nebular Spectroscopy of Nova V906 Carinae

É. J. Harvey, E. Aydi, L. Izzo +7

V906 Carinae was one of the best observed novae of recent times. It was a prolific dust producer and harboured shocks in the early evolving ejecta outflow. Here, we take a close lo…

astro-ph.SR2022★ 10 cited

Modeling the Optical to Ultraviolet Polarimetric Variability from Thomson Scattering in Colliding Wind Binaries

Richard Ignace, Andrew Fullard, Manisha Shrestha +5

Massive star binaries are critical laboratories for measuring masses and stellar wind mass-loss rates. A major challenge is inferring viewing inclination and extracting information…

astro-ph.SR2022

New mass estimates for massive binary systems: a probabilistic approach using polarimetric radiative transfer

Andrew G. Fullard, John T. O'Brien, Wolfgang E. Kerzendorf +4

Understanding the evolution of massive binary stars requires accurate estimates of their masses. This understanding is critically important because massive star evolution can poten…

astro-ph.SR2020★ 10 cited

Polarization simulations of stellar wind bow shock nebulae. II. The case of dust scattering

Manisha Shrestha, Hilding R. Neilson, Jennifer L. Hoffman +2

We study the polarization produced by scattering from dust in a bow shock-shaped region of enhanced density surrounding a stellar source, using the Monte Carlo radiative transfer c…

astro-ph.SR2017★ 11 cited

Polarization simulations of stellar wind bow shock nebulae. I. The case of electron scattering

Manisha Shrestha, Hilding R. Neilson, Jennifer L. Hoffman +1

Bow shocks and related density enhancements produced by the winds of massive stars moving through the interstellar medium provide important information regarding the motions of the…