During an integral-field spectroscopic study of stars in the massive young open cluster NGC 1866 in the Large
Magellanic Cloud, we serendipitously discovered a faint planetary nebula (PN). We designate it “Ka LMC 1,”
and find that its location near the cluster center, along with the agreement of its radial velocity with that of the
cluster, imply a high probability of membership in NGC 1866. The 200 Myr age of the cluster indicates that the
PN’s progenitor star had an initial mass of about 3
The candidates are said to be "published" when they are the object of an official publication in VizieR and in the CDS of the University of Strasbourg.
The Planetary Nebulae .net website offers all the useful and practical information about the planetary nebulae (candidates),
how to apply for a new discovery and how to confirm the candidates. If you would like to contribute to the website, please visit the Data Gathering page and contact us.
Contributors:
Pascal Le Dû - Thomas Petit - Olivier Garde - Nicolas Petit - Trygve Prestgard - Jean-Baptiste Feldmann -
Lionel Mulato - Sakib Rasool - Dana Patchick - Xavier Strottner - Jean-Baptiste Auroux