wpo - session spectra - 2002 Sept 23-30

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2002 Sept 23-30:  A week of observation in poorish transparency.  Some images taken through thin cloud so there are few excuses with spectroscopy!  These lo-res spectra via the SX MX5c single-shot colour camera coupled to a 30cm SCT with the Rainbow transmission grating immediately before the CCD to yield a dispersion of 22A/pixel in exposures from 0.01s for brilliant Vega to 60s for faint variable FI Lyr.  The sessions include exotic Wolf-Rayet emission-line stars in Cygnus/Cepheus posted separately.

All spectra extend into the colourless IR [to right], especially red/IR stars at the bottom of the page, but the visual observer's view is confined principally to the green part of the spectrum  and a little of the blue and red either side.  Photons outside these wavelengths have little effect on the retina.

Double star Albireo [b1Cyg] is an orange K3II star with companion b2Cyg [shown in blue profile] a hotter blue star of spectral type B9.5 like Vega [AOVa] part of the Summer Triangle with Deneb [a Cyg] and Altair [a Aql].  Planet Uranus, with strong methane absorption lines, included below.





The following two shell stars are cooler than WR stars and show emission in Ha, Hb and He.


The trace for cool variables aHer and XY Lyr essentially identical as are the pair FI Lyr and X Oph.



text & images copyright - Maurice Gavin 2002