Search Publications

The Sun's Distance from the Galactic Plane
DOI: 10.1023/B:ASTR.0000005097.18183.64 Bibcode: 2003Ap&SS.288..417B

Branham, R. L., Jr.

Use is made of 93,106 parallaxes from the Hipparcos catalog, with a mixture of spectrum-luminosity classes, to derive the position of the Galactic plane. The reduction technique, mixed total least squares-least squares, takes into account the errors in the parallaxes, and the condition that the direction cosines of the Galactic pole have unit Eucl…

2003 Astrophysics and Space Science
Hipparcos 6
Photometric study of the binary system NN Del
DOI: 10.1023/A:1021324730755 Bibcode: 2003Ap&SS.283..297G

Gómez-Forrellad, J. M.; Sánchez-Bajo, F.; Corbera-Subirana, M. +2 more

We present the results of the differential V light curve analysis of NN Del. We show that NN Del is an EA eclipsing binary system with a period of 99.27 days and a highly eccentric orbit. Photometric solutions obtained using the Russell and the Wilson-Devinney models seem to indicate that both components are very similar in radii and luminosities …

2003 Astrophysics and Space Science
Hipparcos 4
The system of the Milky Way, LMC and SMC
DOI: 10.1023/A:1024068613813 Bibcode: 2003Ap&SS.284..519R

Ružčka, Adam

A simple sticky-particle numerical model has been developed in order to check whether extended structures of gas created due to the dynamical evolution of the Galaxy and the Magellanic Clouds system can be explained as remnants of a tidal interaction. Influence of dissipative nature of gaseous medium has been taken into account. The most remarkabl…

2003 Astrophysics and Space Science
Hipparcos 1
UV Piscium and the Radiative Flux Scale
DOI: 10.1023/A:1021331618901 Bibcode: 2003Ap&SS.283..225V

Vivekananda Rao, P.; Radhika, P.

Studies of eclipsing binaries with Hipparcos parallaxes are found to define a radiative flux relation for main sequence stars in the spectral range from B6 – F0which is about as well as to the stars derived from angular diameters. At lower temperatures the fluxes of the components fall below this curve which is caused due to the large intrinsic va…

2003 Astrophysics and Space Science
Hipparcos 0