Trigonometric parallaxes of 16 nearby planetary nebulae are presented, including reduced errors for seven objects with previous initial results and results for six new objects. The median error in the parallax is 0.42 mas, and twelve nebulae have parallax errors less than 20 percent. The parallax for PHL932 is found here to be smaller than was measured by Hipparcos, and this peculiar object is discussed. Comparisons are made with other distance estimates. The distances determined from these parallaxes tend to be intermediate between some short distance estimates and other long estimates; they are somewhat smaller than estimated from spectra of the central stars. Proper motions and tangential velocities are presented. No astrometric perturba...
We use 612 single stars with previously published trigonometric parallaxes placing them within 25 pc...
Context. Accurate distance measurements are fundamental to the study of planetary nebulae (PNe) but ...
It has recently been noted that the kinematic parallaxes of planetary nebulae (PNe) may be significa...
We present absolute parallaxes and relative proper motions for the central stars of the planetary ne...
By using HIPPARCOS data (magnitudes, parallaxes, proper motions), (1) we determine new values of the...
Original article can be found at: http://www.iop.org/EJ/journal/1538-3881 Copyright American Astrono...
The Hipparcos satellite has measured the parallax of a small sample of planetary nebulae. In this pa...
We have used data obtained with the Fine Guidance Sensors on the Hubble Space Telescope to derive pr...
In this paper we gauge the potentiality of Gala in the distance scale calibration of planetary nebul...
Context. We have compiled a catalogue of central stars of planetary nebulae (CSPN) with reliable dis...
We use the results of our recent NLTE model atmosphere analysis of central stars of old planetary ne...
We report parallax and distance estimates for 12 more cataclysmic binaries and related objects obser...
Aims. We aim to determine individual distances to a small number of rather round, quite regularly sh...
We present trigonometric parallaxes of 64 stellar systems with proper motions between 0.′′5 yr−1 and...
We present absolute trigonometric parallaxes and relative proper motions for three members of the Pl...
We use 612 single stars with previously published trigonometric parallaxes placing them within 25 pc...
Context. Accurate distance measurements are fundamental to the study of planetary nebulae (PNe) but ...
It has recently been noted that the kinematic parallaxes of planetary nebulae (PNe) may be significa...
We present absolute parallaxes and relative proper motions for the central stars of the planetary ne...
By using HIPPARCOS data (magnitudes, parallaxes, proper motions), (1) we determine new values of the...
Original article can be found at: http://www.iop.org/EJ/journal/1538-3881 Copyright American Astrono...
The Hipparcos satellite has measured the parallax of a small sample of planetary nebulae. In this pa...
We have used data obtained with the Fine Guidance Sensors on the Hubble Space Telescope to derive pr...
In this paper we gauge the potentiality of Gala in the distance scale calibration of planetary nebul...
Context. We have compiled a catalogue of central stars of planetary nebulae (CSPN) with reliable dis...
We use the results of our recent NLTE model atmosphere analysis of central stars of old planetary ne...
We report parallax and distance estimates for 12 more cataclysmic binaries and related objects obser...
Aims. We aim to determine individual distances to a small number of rather round, quite regularly sh...
We present trigonometric parallaxes of 64 stellar systems with proper motions between 0.′′5 yr−1 and...
We present absolute trigonometric parallaxes and relative proper motions for three members of the Pl...
We use 612 single stars with previously published trigonometric parallaxes placing them within 25 pc...
Context. Accurate distance measurements are fundamental to the study of planetary nebulae (PNe) but ...
It has recently been noted that the kinematic parallaxes of planetary nebulae (PNe) may be significa...