A deep mosaic of [O III] 5007 A CCD images of the environment of the LBV star P Cygni

Astronomy and Astrophysics – Astrophysics

Scientific paper

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4 pages, 2 figures. Accepted for pubication by A&A Letters

Scientific paper

10.1051/0004-6361:20066039

A mosaic of six, deep, CCD images in the light of the [O III] 5007 A nebular emission line has been obtained with the 1.3-m Skinakas (Crete) telescope of the filamentary nebulosity surrounding P Cygni. The [O III] 5007 A line discriminates against confusing galactic H II regions along the same sight-lines and the new mosaic did not include the 4.8 mag. central star; a source of artifacts in the previous lower angular resolution observations. New giant `lobes' and `shells' are found to be clustered around P Cygni which must be the relics of historic eruptions between 2400 and up to ~10^5 yr ago.

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