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Revealing the dusty shell of the semi-regular variable V CVn
Yanko Nikolov, Nicolaus Steenken, Richard Ignace +8
The semi-regular variable (SRV) star V CVn exhibits a highly variable optical linear polarization, yet its position angle (PA) has remained remarkably stable at approximately 100 +…
Investigating the Light Curves of 5 Long Period Variable Stars: A Study Cross-Harmonics using VStar, MESA, and GYRE
G. M. Sherren, A. Cross, N. Steenken +2
Long Period Variables (LPVs) are Asymptotic Giant Branch stars with periods >100 days. Around one third to half of LPVs display a Long Secondary Period (LSP) that is 5-10 times the…
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…