Add to ORKGWe present the latest results from our study of PNe and HII regions in two Local Group dwarf irregular galaxies IC 10 and NGC 682
We present the first results of our search for new, extended planetary nebulae (PNe) based on carefu...
The chemical abundances of the Galaxy tell us about the stellar and interstellar medium (ISM) evolut...
We present the results of the first spectroscopic observations of two planetary nebula (PN) candidat...
The Local Group (LG) represents the best environment to study in detail the PN population in a large...
Original paper can be found at: http://aspbooks.org/a/volumes Copyright Astronomical Society of the ...
In the framework of the Local Group Census (LGC), a survey of the Local Group (LG) galaxies above De...
Planetary nebulae (PNe) are essential tracers of the kinematics of the diffuse halo and intracluster...
RESUMEN Se analizan datos espectroscópicos de nebulosas planetarias y regiones H II de NGC 3109 y NG...
The Magellanic Clouds are close enough to the Milky Way to provide an excellent environment in which...
Aims. Chemical evolution models are useful for understanding the formation and evolution of stars a...
Up to 10% of the total luminosity of a planetary nebula, ~500 L⊙, can be emitted in the dominant coo...
Planetary Nebulae (PNe) have been used satisfactory to test the effects ofstellar evolution on the G...
International audienceWe compile published spectroscopic data and [O III] magnitudes of almost 500 e...
Our understanding of planetary nebulae has been significantly enhanced as a result of several recent...
The role of planetary nebulae as probes for the galactic chemical evolution is reviewed. Their abund...
We present the first results of our search for new, extended planetary nebulae (PNe) based on carefu...
The chemical abundances of the Galaxy tell us about the stellar and interstellar medium (ISM) evolut...
We present the results of the first spectroscopic observations of two planetary nebula (PN) candidat...
The Local Group (LG) represents the best environment to study in detail the PN population in a large...
Original paper can be found at: http://aspbooks.org/a/volumes Copyright Astronomical Society of the ...
In the framework of the Local Group Census (LGC), a survey of the Local Group (LG) galaxies above De...
Planetary nebulae (PNe) are essential tracers of the kinematics of the diffuse halo and intracluster...
RESUMEN Se analizan datos espectroscópicos de nebulosas planetarias y regiones H II de NGC 3109 y NG...
The Magellanic Clouds are close enough to the Milky Way to provide an excellent environment in which...
Aims. Chemical evolution models are useful for understanding the formation and evolution of stars a...
Up to 10% of the total luminosity of a planetary nebula, ~500 L⊙, can be emitted in the dominant coo...
Planetary Nebulae (PNe) have been used satisfactory to test the effects ofstellar evolution on the G...
International audienceWe compile published spectroscopic data and [O III] magnitudes of almost 500 e...
Our understanding of planetary nebulae has been significantly enhanced as a result of several recent...
The role of planetary nebulae as probes for the galactic chemical evolution is reviewed. Their abund...
We present the first results of our search for new, extended planetary nebulae (PNe) based on carefu...
The chemical abundances of the Galaxy tell us about the stellar and interstellar medium (ISM) evolut...
We present the results of the first spectroscopic observations of two planetary nebula (PN) candidat...