i. On the relation of mean stellar parallax to proper motion and apparent magnitude • ii. On the progression of stellar velocity with absolute magnitude • iii. Mean absolute magnitude of a group of stars. (Note on a paper by Messrs. Young and Harper). • iv. On the numerical solution of integral equation
Since the first successful measurements of stellar trigonometric parallax in the 1830s, the study of...
Astrometric measurements of microlensing events can in principle determine both the "parallax" r_E a...
A new value for the absolute proper motion of the R CrB type variable star U Aqr has been derived on...
We compare the absolute visual magnitude of the majority of bright O stars in the sky as predicted f...
The mean absolute magnitude of the Am stars was determined from statistical parallaxes. The material...
R. R. La parallaxe moyenne des étoiles et le mouvement du système solaire. Newcomb S. — Some points ...
Bienayme et al. (1992) have published a magnitude-limited sample of proper motions for stars at the ...
Since the first successful measurements of stellar trigonometric parallax in the 1830s, the study of...
We present a new procedure for photometric parallax estimation. The data for 1236 stars provide cali...
The methods of secular and statistical parallax for homogeneous groups of Galactic stars are applied...
As a preliminary step to derive the luminosity function the underlying hypothesis involved in the me...
The solar motion and the velocity ellipsoid are derived from samples of stars of different spectral ...
In this paper we investigate whether a misestimate of proper motions could have been a source of sub...
The theoretical prediction that trigonometric parallaxes suffer from a statistical effect, has becom...
The MEarth survey is a search for small rocky planets around the smallest, nearest stars to the Sun ...
Since the first successful measurements of stellar trigonometric parallax in the 1830s, the study of...
Astrometric measurements of microlensing events can in principle determine both the "parallax" r_E a...
A new value for the absolute proper motion of the R CrB type variable star U Aqr has been derived on...
We compare the absolute visual magnitude of the majority of bright O stars in the sky as predicted f...
The mean absolute magnitude of the Am stars was determined from statistical parallaxes. The material...
R. R. La parallaxe moyenne des étoiles et le mouvement du système solaire. Newcomb S. — Some points ...
Bienayme et al. (1992) have published a magnitude-limited sample of proper motions for stars at the ...
Since the first successful measurements of stellar trigonometric parallax in the 1830s, the study of...
We present a new procedure for photometric parallax estimation. The data for 1236 stars provide cali...
The methods of secular and statistical parallax for homogeneous groups of Galactic stars are applied...
As a preliminary step to derive the luminosity function the underlying hypothesis involved in the me...
The solar motion and the velocity ellipsoid are derived from samples of stars of different spectral ...
In this paper we investigate whether a misestimate of proper motions could have been a source of sub...
The theoretical prediction that trigonometric parallaxes suffer from a statistical effect, has becom...
The MEarth survey is a search for small rocky planets around the smallest, nearest stars to the Sun ...
Since the first successful measurements of stellar trigonometric parallax in the 1830s, the study of...
Astrometric measurements of microlensing events can in principle determine both the "parallax" r_E a...
A new value for the absolute proper motion of the R CrB type variable star U Aqr has been derived on...