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26 April 2024
 
  » arxiv » astro-ph/0301129

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Spectroscopy of planetary nebulae in M33
L. Magrini ; M. Perinotto ; R.L.M. Corradi ; A. Mampaso ;
Date 8 Dec 2002
Journal Astron.Astrophys. 400 (2003) 511-520
Subject astro-ph
AffiliationDipartimento di Astronomia e Scienza dello Spazio, Firenze Isaac Newton Group of Telescopes, La Palma, Spain Instituto de Astrofisica de Canarias, Tenerife, Spain
AbstractSpectroscopic observations of 48 emission-line objects of M33 have been obtained with the multi-object, wide field, fibre spectrograph AF2/WYFFOS at the 4.2m WHT telescope (La Palma, Spain). Line intensities and logarithmic extinction, cbeta, are presented for 42 objects. Their location in the Sabbadin & D’Odorico diagnostic diagram (Halpha/[SII] vs Hlapha/[NII]) suggests that >70% of the candidates are Planetary Nebulae (PNe). Chemical abundances and nebular physical parameters have been derived for the three of the six PNe where the 4363A [OIII] emission line was measurable. These are disc PNe, located within a galactocentric distance of 4.1 kpc, and, to date, they are the farthest PNe with a direct chemical abundance determination. No discrepancy in the Helium, Oxygen and Argon abundances has been found in comparison with corresponding abundances of PNe in our Galaxy. Only a lower limit to the sulphur abundance has been obtained since we could not detect any [SIII] line. N/H appears to be lower than the Galactic value; some possible explanations for this under-abundance are discussed.
Source arXiv, astro-ph/0301129
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