Volume 367, Number 2, February IV 2001
|Page(s)||498 - 500|
|Section||Cosmology (including clusters of galaxies)|
|Published online||15 February 2001|
Accurate positions of candidate planetary nebulae in M 33
Dipartimento di Astronomia e Scienza dello Spazio, Università di Firenze, L.go E. Fermi 5, 50125 Firenze, Italy
2 Instituto de Astrofísica de Canarias, c. Vía Láctea s/n, 38200, La Laguna, Tenerife, Spain
3 Department of Physics and Astronomy, The Open University, Milton Keynes MK7 6AA, UK
4 Isaac Newton Group of Telescopes, Apartado de Correos 321, 38700 Santa Cruz de la Palma, Spain
Corresponding author: M. Perinotto, firstname.lastname@example.org
Accepted: 12 December 2000
We present new determinations of the positions of the planetary nebulae candidates found in Messier 33 by Magrini et al. (2000). The new coordinates have an accuracy of ±0.3 arcsec, making them suitable for future studies of the individual objects by means of, for instance, multi-object fiber or slit spectroscopy.
Key words: planetary nebulae / galaxies: M 33
© ESO, 2001
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