Add to ORKGThe luminosity of the central stars planetary nebulas near the galactic center is discussed. The distance to these objects is quite well known, removing the most common source of uncertainty in luminosity determinations. The resulting luminosities are compared to theoretical models and to empirical determinations from nearby nebulas using different method
The increase in discovered close binary central stars of planetary nebulae is leading to a sufficien...
We surveyed the central $4 \times 4$ degrees of the Galactic center for planetary nebulae in the lig...
Context. In recent years mid-and far infrared spectra of planetary nebulae have been analysed and le...
The luminosity of the central stars planetary nebulas near the galactic center is discussed. The dis...
Luminosity functions for planetary nebulae in the galactic bulge and the Magellanic Clouds are prese...
Context.Optical high-resolution spectra of five central stars of planetary nebulae (CSPN) in the Gal...
Using existing infrared and radio data on a sample of 432 planetary nebulae, we have derived a numbe...
The position of the central stars of planetary nebulae on the T/L diagram provides an important test...
International audienceAims: We present a homogeneous set of spectroscopic measurements secured with ...
Context. We have compiled a catalogue of central stars of planetary nebulae (CSPN) with reliable dis...
Context.The luminosity function of planetary nebulae, in use for about two decades in extragalactic...
Aims. We present a homogeneous set of spectroscopic measurements secured with 4-m class telescopes f...
For a sample of 23 Galactic planetary nebulae, selected on the basis of distance certainty and tempe...
We propose to use the correlation between the distance-independent radio continuum brightness temper...
Aims. The evolution of central stars of planetary nebulae was so far documented in just a few cases....
The increase in discovered close binary central stars of planetary nebulae is leading to a sufficien...
We surveyed the central $4 \times 4$ degrees of the Galactic center for planetary nebulae in the lig...
Context. In recent years mid-and far infrared spectra of planetary nebulae have been analysed and le...
The luminosity of the central stars planetary nebulas near the galactic center is discussed. The dis...
Luminosity functions for planetary nebulae in the galactic bulge and the Magellanic Clouds are prese...
Context.Optical high-resolution spectra of five central stars of planetary nebulae (CSPN) in the Gal...
Using existing infrared and radio data on a sample of 432 planetary nebulae, we have derived a numbe...
The position of the central stars of planetary nebulae on the T/L diagram provides an important test...
International audienceAims: We present a homogeneous set of spectroscopic measurements secured with ...
Context. We have compiled a catalogue of central stars of planetary nebulae (CSPN) with reliable dis...
Context.The luminosity function of planetary nebulae, in use for about two decades in extragalactic...
Aims. We present a homogeneous set of spectroscopic measurements secured with 4-m class telescopes f...
For a sample of 23 Galactic planetary nebulae, selected on the basis of distance certainty and tempe...
We propose to use the correlation between the distance-independent radio continuum brightness temper...
Aims. The evolution of central stars of planetary nebulae was so far documented in just a few cases....
The increase in discovered close binary central stars of planetary nebulae is leading to a sufficien...
We surveyed the central $4 \times 4$ degrees of the Galactic center for planetary nebulae in the lig...
Context. In recent years mid-and far infrared spectra of planetary nebulae have been analysed and le...