Poster abstract details
Sh 2-71 and its possible binary central star
Abstract
We present new observations of the remarkable planetary nebula SH 2-71.
Deep Halpha+[NII] images allow the detection of faint extensions of the radial structures observed in the inner regions of the nebula.
The properties of the two candidate central stars of the nebula are also discussed by means of time-series spectroscopy and new photometry.
Deep Halpha+[NII] images allow the detection of faint extensions of the radial structures observed in the inner regions of the nebula.
The properties of the two candidate central stars of the nebula are also discussed by means of time-series spectroscopy and new photometry.