Contenidos
Imágenes
Subir su imagen
DSS Images Other Images
Artículos relacionados
Kinematics of Hipparcos Visual Binaries. II. Stars with Ground-Based Orbital Solutions This paper continues kinematical investigations of the Hipparcos visualbinaries with known orbits. A sample, consisting of 804 binary systemswith orbital elements determined from ground-based observations, isselected. The mean relative error of their parallaxes is about 12% andthe mean relative error of proper motions is about 4%. However, even 41%of the sample stars lack radial velocity measurements. The computedGalactic velocity components and other kinematical parameters are usedto divide the stars with known radial velocities into kinematical agegroups. The majority (92%) of binaries from the sample are thin diskstars, 7.6% have thick disk kinematics and only two binaries have halokinematics. Among them, the long-period variable Mira Ceti has a verydiscordant {Hipparcos} and ground-based parallax values. From the wholesample, 60 stars are ascribed to the thick disk and halo population.There is an urgent need to increase the number of the identified halobinaries with known orbits and substantially improve the situation withradial velocity data for stars with known orbits.
| Observations of Double Stars. XVIII. Micrometer observations of 1350 pairs in 1995-1997 are listed.
| ICCD Speckle Observations of Binary Stars. XIII. Measurements During 1989- 1994 From the Cerro Tololo 4 M Telescope Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1996AJ....111..936H&db_key=AST
| UBV photometry of HD stars in the fields of selected cataclysmic variables. Not Available
| Micrometer observations of double stars and new pairs. XIII From a program of double star observations which emphasizes orbital,neglected, and newly discovered pairs, results obtained from October1984 to January 1987 are presented. A total of 3030 visual and 550photographic measures are listed. The positions in WDS format andDurchmusterung numbers are shown for 117 pairs for which firstobservations appear in this paper. Magnitudes are estimated for some ofthe objects.
| Rotational velocities of faint stars of early spectral types. Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1963AJ.....68..428S&db_key=AST
|
Enviar un nuevo artículo
Enlaces relacionados
- - No se han encontrado enlaces -
En viar un nuevo enlace
Miembro de los siguientes grupos:
|
Datos observacionales y astrométricos
Constelación: | Ballena |
Ascensión Recta: | 00h12m33.16s |
Declinación: | -11°41'34.7" |
Magnitud Aparente: | 8.16 |
Distancia: | 185.529 parsecs |
Movimiento Propio en Ascensión Recta: | 2.1 |
Movimiento Propio en Declinación: | -2.2 |
B-T magnitude: | 8.561 |
V-T magnitude: | 8.194 |
Catálogos y designaciones:
|