Add to ORKGWe have proposed a statistical method to determine distances to planetary nebulae. The method is based on an empirical correlation between the radio-continuum brightness temperature and radius. Here we present a catalog of distance determinations calculated using this method.</p
We use the results of our recent NLTE model atmosphere analysis of central stars of old planetary ne...
This investigation had two main purposes. The first was to determine individual distances of a numbe...
Context. We have compiled a catalogue of central stars of planetary nebulae (CSPN) with reliable dis...
We have proposed a statistical method to determine distances to planetary nebulae. The method is bas...
We have proposed a statistical method to determine distances to planetary nebulae. The method is bas...
We propose to use the correlation between the distance-independent radio continuum brightness temper...
By collecting distances from the literature, a set of 73 planetarynebulae with mean distances of hig...
We have developed a self-consistent method to determine the physical parameters of planetary nebulae...
At present the lack of a good, generally accepted distance scare is the major limitation in the stud...
Context. The advent of large-scale, high-sensitivity surveys of the Galaxy (2MASS, WISE, Spitzer, et...
Measuring the distances to Galactic planetary nebulae (PNe) has been an intractable problem for many...
Measuring the distances to Galactic planetary nebulae (PNe) has been an intractable problem for many...
Abstract. We use the results of our recent NLTE model atmosphere analysis of central stars of old pl...
We report the results of [OIII] lambda 5007 surveys for planetary nebulae (PNe) in NGC 2403, 3115, 3...
The local planetary nebula (PN) census is dominated by extremely evolved examples, and until recentl...
We use the results of our recent NLTE model atmosphere analysis of central stars of old planetary ne...
This investigation had two main purposes. The first was to determine individual distances of a numbe...
Context. We have compiled a catalogue of central stars of planetary nebulae (CSPN) with reliable dis...
We have proposed a statistical method to determine distances to planetary nebulae. The method is bas...
We have proposed a statistical method to determine distances to planetary nebulae. The method is bas...
We propose to use the correlation between the distance-independent radio continuum brightness temper...
By collecting distances from the literature, a set of 73 planetarynebulae with mean distances of hig...
We have developed a self-consistent method to determine the physical parameters of planetary nebulae...
At present the lack of a good, generally accepted distance scare is the major limitation in the stud...
Context. The advent of large-scale, high-sensitivity surveys of the Galaxy (2MASS, WISE, Spitzer, et...
Measuring the distances to Galactic planetary nebulae (PNe) has been an intractable problem for many...
Measuring the distances to Galactic planetary nebulae (PNe) has been an intractable problem for many...
Abstract. We use the results of our recent NLTE model atmosphere analysis of central stars of old pl...
We report the results of [OIII] lambda 5007 surveys for planetary nebulae (PNe) in NGC 2403, 3115, 3...
The local planetary nebula (PN) census is dominated by extremely evolved examples, and until recentl...
We use the results of our recent NLTE model atmosphere analysis of central stars of old planetary ne...
This investigation had two main purposes. The first was to determine individual distances of a numbe...
Context. We have compiled a catalogue of central stars of planetary nebulae (CSPN) with reliable dis...