Celestial hemisphere:  Northern  ·  Constellation: Cepheus (Cep)  ·  Contains:  HD211746  ·  PK107+07.1
Getting plate-solving status, please wait...
IsWe2 (Ishida-Weinberger 2), James E.
Powered byPixInsight

IsWe2 (Ishida-Weinberger 2)

Getting plate-solving status, please wait...
IsWe2 (Ishida-Weinberger 2), James E.
Powered byPixInsight

IsWe2 (Ishida-Weinberger 2)

Equipment

Loading...

Acquisition details

Loading...

Description

Ishida Weinberger 2 (IW2 or IsWe2) is a large, ancient planetary nebula in Cepheus and is about 850 light years distant (K. Ishida and R. Weinberger, “Two senile nearby planetary nebula and the local PN population,” Astronomy and Astrophysics, 178, 227-236, 1987). It appears to be slightly elongated in the NW-SE direction encompassing about 18.5’. From the expansion velocities of Ha and NII, IW 2 is estimated to have a kinematic age of about 40000 years. It is quite faint but emits both Ha and NII [but no detectable OIII with our equipment]. The effective temperature of its white dwarf star is 100,000 K.  It is one of the larger PN known being nearly 4 light years in extent. The filamentary structures are likely shock fronts due to the nebula interacting with the interstellar medium. The central star, situated near the “S” shaped filament, is clearly displaced from the geometrical center of the nebula, (K. M. Xilouris et al., “The shaping of aging planetary nebulae,” Astronomy and Astrophysics, 310, 603-612, 1996).   [ref:  Astrodon Imaging, IW2, 2011] 

This PN is basically an Ha-only target (and NII according to professional sources) with no OIII data present.  Drawing out the faint structure of this planetary nebula also revealed an abundance of superimposed Ha which made this target essentially blend in with background. 

Imaged over several nights:  Sept 14-18, and 24, 2020.

Comments