We estimate distances to the spherical planetary nebula Abell 39 and the bipolar planetary nebula NGC 7027 by interpolating from a wide grid of photoionization models using the 3-D code, MOCASSIN. We find preliminary distances of 1.5 kpc and 0.9 kpc respectively, with uncertainties of about 30%.link_to_subscribed_fulltex
Abstract. We use the results of our recent NLTE model atmosphere analysis of central stars of old pl...
Context. Individual distances to planetary nebulae are of the utmost relevance for our understanding...
We propose to use the correlation between the distance-independent radio continuum brightness temper...
We present the results of a study of the planetary nebula NGC 40 with the use of the 3-D photoioniza...
Continuing our series of papers on the three-dimensional (3D) structure and accurate distances of pl...
We have developed a self-consistent method to determine the physical parameters of planetary nebulae...
The three-dimensional Monte Carlo photoionization code Mocassin has been applied to con-struct a rea...
At present the lack of a good, generally accepted distance scare is the major limitation in the stud...
We present the results of a spatio-kinematic study of the planetary nebula Menzel 1 using spectro-ph...
Context. The advent of large-scale, high-sensitivity surveys of the Galaxy (2MASS, WISE, Spitzer, et...
Aims. We aim to determine individual distances to a small number of rather round, quite regularly sh...
Aims. We present a coherent stellar and nebular model that reproduces observations of the planetary ...
We present individual distances to three PNe: NGC 6537, NGC 6781 and NGC 7027, determined by the ext...
We have constructed photoionization models of five galactic bulge planetary nebulae using our automa...
We have proposed a statistical method to determine distances to planetary nebulae. The method is bas...
Abstract. We use the results of our recent NLTE model atmosphere analysis of central stars of old pl...
Context. Individual distances to planetary nebulae are of the utmost relevance for our understanding...
We propose to use the correlation between the distance-independent radio continuum brightness temper...
We present the results of a study of the planetary nebula NGC 40 with the use of the 3-D photoioniza...
Continuing our series of papers on the three-dimensional (3D) structure and accurate distances of pl...
We have developed a self-consistent method to determine the physical parameters of planetary nebulae...
The three-dimensional Monte Carlo photoionization code Mocassin has been applied to con-struct a rea...
At present the lack of a good, generally accepted distance scare is the major limitation in the stud...
We present the results of a spatio-kinematic study of the planetary nebula Menzel 1 using spectro-ph...
Context. The advent of large-scale, high-sensitivity surveys of the Galaxy (2MASS, WISE, Spitzer, et...
Aims. We aim to determine individual distances to a small number of rather round, quite regularly sh...
Aims. We present a coherent stellar and nebular model that reproduces observations of the planetary ...
We present individual distances to three PNe: NGC 6537, NGC 6781 and NGC 7027, determined by the ext...
We have constructed photoionization models of five galactic bulge planetary nebulae using our automa...
We have proposed a statistical method to determine distances to planetary nebulae. The method is bas...
Abstract. We use the results of our recent NLTE model atmosphere analysis of central stars of old pl...
Context. Individual distances to planetary nebulae are of the utmost relevance for our understanding...
We propose to use the correlation between the distance-independent radio continuum brightness temper...