Results 71 to 80 of about 207,371 (176)
Planetary Nebulae surveys: Past, Present and Future
In this review we cover the detection, identification and astrophysical importance of planetary nebulae (PN). The legacy of the historic Perek & Kohoutek and Acker et al.
Frew, DJ, Parker, QA
core
Planetary nebulae in the Magellanic Clouds
Context.We present the second part of an optical spectroscopic study of planetary nebulae in the ...
P. Leisy +3 more
core +1 more source
MUSE imaging spectroscopy of the fullerene planetary nebula Tc 1
Aims. The planetary nebula Tc 1 (PN G345.2–08.8), one of the rare group of Galactic PNe showing fullerene emission in the infrared, is spatially extended with high a surface brightness.
Walsh J. R. +8 more
doaj +1 more source
New Close Binary Central Stars of Planetary Nebulae from Gaia DR3 Epoch Photometry. [PDF]
Chornay N, Walton NA.
europepmc +1 more source
Planetary Nebulae in the Solar Neighborhood (poster)
Poster presented at "Planetary Nebulae as Astronomical Tools" Conference, Gdansk, Poland ...
David Frew (764192) +1 more
core +1 more source
Whither or Wither the Sulfur Anomaly in Planetary Nebulae?
We present a thorough investigation of the long-standing sulfur anomaly enigma. Our analysis uses chemical abundances from the most extensive data set available for 126 planetary nebulae (PNs) with improved accuracy and reduced uncertainties from a 10° ×
Shuyu Tan, Quentin A. Parker
doaj +1 more source
Chemical abundances in seven galactic planetary nebulae
An observational study of chemical abundances in the galactic planetary nebulae NGC ...
M. V. F. Copetti, A. C. Krabbe
core +1 more source
Close Binaries and the Abundance Discrepancy Problem in Planetary Nebulae
Motivated by the recent establishment of a connection between central star binarity and extreme abundance discrepancies in planetary nebulae, we have carried out a spectroscopic survey targeting planetary nebula with binary central stars and previously ...
R. Wesson +4 more
doaj +1 more source
A new [OIII] lambda5007 Å Galactic Planetary Nebulae Luminosity Function
The Planetary Nebulae Luminosity Function (PNLF) describes the collective luminosity evolution for a given population of Planetary Nebulae (PN). A major paradox in current PNLF studies is in the universality of the absolute magnitude of the brightest PNe
Miszalski, B +3 more
core
The temperature structure of dusty planetary nebulae
We have analyzed the effects of photoelectric heating by dust grains in photoionization models of planetary nebulae. We have shown that this process is particularly important if planetary nebulae contain a population of small grains. The presence of such
G. Stasińska, R. Szczerba
core +1 more source

