Abstract. New observations and derived chemical abundances are reported for a sample of 57 bulge planetary nebulae (PN). Together with our previous results, a total of over a hundred objects have been analyzed, which constitute one of the largest samples of bulge nebulae studied under homogeneous conditions, including equipment and reduction procedures. In general, our data show a good agreement with some recent results in the literature, in the sense that the average abundances of bulge PN are similar to those from disk objects, however showing a larger dispersion. Key words. planetary nebulae: general – galaxies: bulges – techniques: spectroscopi
Context. Our understanding of the chemical evolution (CE) of the Galactic bulge requires the determi...
We present mid-infrared Spitzer spectra of 11 planetary nebulae in the Galactic bulge. We derive arg...
We present mid-infrared Spitzer spectra of 11 planetary nebulae in the Galactic bulge. We derive arg...
New observations and derived chemical abundances are reported for a sample of 57 bulge planetary neb...
New observations and derived chemical abundances are reported for a sample of 57 bulge planetary neb...
International audienceWe have observed 44 planetary nebulae (PNe) in the direction of the Galactic b...
International audienceWe have observed 44 planetary nebulae (PNe) in the direction of the Galactic b...
International audienceWe have observed 44 planetary nebulae (PNe) in the direction of the Galactic b...
The abundances of the planetary nebulae (PNe) in the galactic bulge are presented. Comparisons are m...
Context. Our understanding of the chemical evolution (CE) of the Galactic bulge requires the determi...
The abundances of the planetary nebulae (PNe) in the galactic bulge are presented. Comparisons are m...
Context. Planetary nebulae (PNe) abundances are poorly known for those nebulae in the Galactic bulge...
Context. Planetary nebulae (PNe) abundances are poorly known for those nebulae in the Galactic bulge...
Context. Planetary nebulae (PNe) abundances are poorly known for those nebulae in the Galactic bulge...
We discuss discovery of a new population of up to 300 planetary nebulae (PNe) candidates captured se...
Context. Our understanding of the chemical evolution (CE) of the Galactic bulge requires the determi...
We present mid-infrared Spitzer spectra of 11 planetary nebulae in the Galactic bulge. We derive arg...
We present mid-infrared Spitzer spectra of 11 planetary nebulae in the Galactic bulge. We derive arg...
New observations and derived chemical abundances are reported for a sample of 57 bulge planetary neb...
New observations and derived chemical abundances are reported for a sample of 57 bulge planetary neb...
International audienceWe have observed 44 planetary nebulae (PNe) in the direction of the Galactic b...
International audienceWe have observed 44 planetary nebulae (PNe) in the direction of the Galactic b...
International audienceWe have observed 44 planetary nebulae (PNe) in the direction of the Galactic b...
The abundances of the planetary nebulae (PNe) in the galactic bulge are presented. Comparisons are m...
Context. Our understanding of the chemical evolution (CE) of the Galactic bulge requires the determi...
The abundances of the planetary nebulae (PNe) in the galactic bulge are presented. Comparisons are m...
Context. Planetary nebulae (PNe) abundances are poorly known for those nebulae in the Galactic bulge...
Context. Planetary nebulae (PNe) abundances are poorly known for those nebulae in the Galactic bulge...
Context. Planetary nebulae (PNe) abundances are poorly known for those nebulae in the Galactic bulge...
We discuss discovery of a new population of up to 300 planetary nebulae (PNe) candidates captured se...
Context. Our understanding of the chemical evolution (CE) of the Galactic bulge requires the determi...
We present mid-infrared Spitzer spectra of 11 planetary nebulae in the Galactic bulge. We derive arg...
We present mid-infrared Spitzer spectra of 11 planetary nebulae in the Galactic bulge. We derive arg...