A planetary nebula is the remnant of a former red-giant where the ejected outer layers fluoresce under the intense UV radiation from the exposed stellar remnant core. PNe are relatively easy to record via the spectroscope because all their light is concentrated in a few emission lines rather than being dissipated into the background continuum like a star - twin oxygen lines (OIII~500nm in green) is usually the most prominent with Ha(red) then Hb(blue) less so.my homepage main spectroscopy page novae in Aquila [similar spectra] ELCAT PNe complete list - galactic+intergalactic
2003 Dec: PNe NGC 2371/2 [Gem] and repeat NGC 2022 [Ori].![]()
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2003 Feb: Three winter PNe ie IC 2165 [CMa @ -13o Dec], NGC 2022 [Ori] and Eskimo [Gem].
Other VS stars etc during observing sessions here.![]()
2002 July 18/19/25: A productive week of elusive summer PNe spectra some through haze with a lvm 2 but CCDs punch through the most demanding skies!
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2000 June 11: Very poor conditions - strong cirrus + gibbous moon; lvm ~2.5 but this starlike PNe PK82+11.1 = NGC 6833 in Cygnus recorded. Sky Cat 2000 quotes RA 19h 49.7m; Dec +48o 58'; 1"diam; m[pg]13.8. The spectra seems classic i.e. unresolved duo of OIII ~500nm dominates with Ha strong and Hb abutting OIII distinct plus very weak line[s] in violet in this spectrum with red to the left.![]()
1999 Aug 19: amongst the brightest of planetaries - the Blue Snowball [NGC 7662] targeted in And. At the Ewell AS next evening it appears a vivid blue non-stellar disk through a member's Meade 9cm ETX/EC [nice 'scope]. A reworked spectrum via the OG prism is included.
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1999 June 24/25 - M57 captured during stellar spectra session in Lyra plus my favourite near stellar PNe in adjacent Hercules.
Sky Cat 2000 quotes [p312] PK51+9.1 @ RA18h 49.7' Dec+20o 51'; Her; 3" diam; m[pg] 12.2; central star mv13? WR spect; dist 1.3kpc
Hu2-1 51+09 1 VV208 or VV458, Type III PN MD92. Star-like PN extract from ELCAT PNe complete list
Hu2-1 51+09 1 IRAS18476+2047 NOS4_2. Relatively low-excit PN
Hu2-1 51+09 1 G51.4+9.6 LU4_2. Compact PN KA93.
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The following near 'stellar' PNe spectra captured Aug/Sept'98 via 30cm SCT+Mk1a (dv-prism) spectroscope working @ f/3.5 i.e. 1m focal length. The ratio of OIII (oxygen), hydrogen and helium emission lines remain similar throughout the series. Campbell's Star [not shown] is the exception - lines positions normally allocated to hydrogen are attributed to ionised helium - He I as for WR stars - planetary stellar core [if recorded] have typically WR spectra.
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text & images copyright - Maurice Gavin - WPO 1998 -2003