NGC281 in L(Ha)SHO

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NGC281 in SHO narrowband palette, with Ha integrated as Luminance layer, as according to to Nik Szymanek approach to Sulphur-II Luminance Compositing.

Ha layer (luminosity blending) added in starless and stars separate layers.

SHO stunning integration

Data recorded by Officina Stellare ProRC 700 and QHY 600M CMOS, subframes at 120sec, -5 C, from IC Observatory of Spain, telescopelive network.

Astrobin: https://www.astrobin.com/2f69ta/B/

NGC281 SHO palette

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NGC281 in SHO palette, crop to focus about Pacman Nebula.

Deep reworking focused about colors and histogram stretching over integration obtained by several records in SHO narrowband by William Optics Redcat 51, ASI1600mm on EQM35 collected between 2021 and this year.

Original wider field

Astrobin:

NGC6960 “Veil Nebula” in SHO

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NGC6960 “Veil Nebula” in SHO palette; subframes of 180″ recorded by ASI1600mm Pro on W.O. Redcat 51, mount EQM35 Pro, from 6 degrees Bortle scale suburban sky of Livorno city (IT).

In modern usage, the names Veil Nebula, Cirrus Nebula, and Filamentary Nebula generally refer to all the visible structure of a Supernova remnant, or even to the entire loop itself; this structure is so large that several NGC numbers were assigned to various arcs of the nebula.

Astrobin: https://www.astrobin.com/bskbi3/