Add to ORKGThe solar motion and the velocity ellipsoid are derived from samples of stars of different spectral types and luminosity class. The equations used are those of the radial velocity component of motion, including the K-term and galactic rotation corrections. The results obtained are compared with the published ones. The complete paper will be published elsewhere.Asociación Argentina de Astronomí
The distribution and motions of both neutral and ionized hydrogen can be studied throughout the Gala...
The kinematic properties of gas and stars in the solar neighbourhood are described in terms of the l...
van Rhijn’s method is used to derive the luminosity function in the solar neighbourhood from large p...
The solar motion and the velocity ellipsoid are derived from samples of stars of different spectral ...
As a preliminary step to derive the luminosity function the underlying hypothesis involved in the me...
It has been studied the formation of the continuum of nebular hydrogen when ionization is due to rad...
hrough a convenient model, it is shown that galaxies with a condensed nuclear body breaking in two p...
We analyse the kinematics of ~400 000 stars that lie within ̃2 kpc of the Sun and have spectra measu...
The high-velocity hydrogen clouds at high latitudes have been widely discussed as material falling i...
We analyse the kinematics of ˜400 000 stars that lie within ˜2 kpc of the Sun and have spectra measu...
The apparent radial velocity of a star, as deduced from wavelength shifts, comprises not merely its ...
We analyse the kinematics of ∼400 000 stars that lie within ∼2 kpc of the Sun and have spectra measu...
Context. The velocity distribution of stars in the solar neighbourhood is inhomogeneous and rich wit...
We analyse the kinematics of ~400000 RAVE stars. We split the sample into hot and cold dwarfs, red-c...
Looking up, at night, one can immediately notice that the universe is almost empty. On a bright nigh...
The distribution and motions of both neutral and ionized hydrogen can be studied throughout the Gala...
The kinematic properties of gas and stars in the solar neighbourhood are described in terms of the l...
van Rhijn’s method is used to derive the luminosity function in the solar neighbourhood from large p...
The solar motion and the velocity ellipsoid are derived from samples of stars of different spectral ...
As a preliminary step to derive the luminosity function the underlying hypothesis involved in the me...
It has been studied the formation of the continuum of nebular hydrogen when ionization is due to rad...
hrough a convenient model, it is shown that galaxies with a condensed nuclear body breaking in two p...
We analyse the kinematics of ~400 000 stars that lie within ̃2 kpc of the Sun and have spectra measu...
The high-velocity hydrogen clouds at high latitudes have been widely discussed as material falling i...
We analyse the kinematics of ˜400 000 stars that lie within ˜2 kpc of the Sun and have spectra measu...
The apparent radial velocity of a star, as deduced from wavelength shifts, comprises not merely its ...
We analyse the kinematics of ∼400 000 stars that lie within ∼2 kpc of the Sun and have spectra measu...
Context. The velocity distribution of stars in the solar neighbourhood is inhomogeneous and rich wit...
We analyse the kinematics of ~400000 RAVE stars. We split the sample into hot and cold dwarfs, red-c...
Looking up, at night, one can immediately notice that the universe is almost empty. On a bright nigh...
The distribution and motions of both neutral and ionized hydrogen can be studied throughout the Gala...
The kinematic properties of gas and stars in the solar neighbourhood are described in terms of the l...
van Rhijn’s method is used to derive the luminosity function in the solar neighbourhood from large p...