Discovery of a narrow constant-width H-alpha trail in the Cygnus Loop, interpreted as a Balmer-dominated non-radiative shock from the SNR encountering dense material or magnetic structure edge-on.
The Astrophysical Journal , abstract =
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New SBF distance confirms NGC5846_UDG1 lies in the NGC 5846 group and reconciles prior GC counts to ~50 members, supporting a massive dark matter halo.
citing papers explorer
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Discovery of an extremely narrow trail-like feature crossing the Veil Supernova Remnant in deep amateur observations
Discovery of a narrow constant-width H-alpha trail in the Cygnus Loop, interpreted as a Balmer-dominated non-radiative shock from the SNR encountering dense material or magnetic structure edge-on.
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Revisiting the distance and the globular cluster system of the remarkable galaxy UDG1 in the NGC 5846 group
New SBF distance confirms NGC5846_UDG1 lies in the NGC 5846 group and reconciles prior GC counts to ~50 members, supporting a massive dark matter halo.