Zobrazeno 1 - 7
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pro vyhledávání: '"Collaboration, the RAVE"'
The 5th RAVE data release is based on 520,781 spectra ($R\approx7500$ in the CaT region at $8410$ - $8795$\AA) of 457,588 unique stars. RAVE DR5 provides radial velocities, stellar parameters and individual abundances for up to seven elements and dis
Externí odkaz:
http://arxiv.org/abs/1710.08559
Autor:
C., Boeche, collaboration, the RAVE
RAVE is a spectroscopic survey of the Milky Way which collected more than 500,000 stellar spectra of nearby stars in the Galaxy. The RAVE consortium analysed these spectra to obtain radial velocities, stellar parameters and chemical abundances. These
Externí odkaz:
http://arxiv.org/abs/1309.6460
With the advent of the Gaia data, the unprecedented kinematic census of great part of the Milky Way disc will allow us to characterise the local kinematic groups and new groups in different disc neighbourhoods. First, we show here that the models pre
Externí odkaz:
http://arxiv.org/abs/1110.5907
Although primarily aimed at the galactic archeology and evolution, automated all-sky spectroscopic surveys (RAVE, SDSS) are also a valuable source for the binary star research community. Identification of double-lined spectra is easy and it is not li
Externí odkaz:
http://arxiv.org/abs/0910.1222
The Arcturus moving group is a well-populated example of phase space substructure within the thick disk of our Galaxy. Traditionally regarded as the remains of a dissolved open cluster, it has recently been suggested to be a remnant of a satellite ac
Externí odkaz:
http://arxiv.org/abs/0810.2669
Autor:
Siebert, A., collaboration, the RAVE
RAVE, the RAdial Velocity Experiment, is an ambitious program to conduct a survey to measure the radial velocities, metallicities and abundance ratios for up to a million stars using the 1.2-m UK Schmidt Telescope of the Anglo-Australian Observatory
Externí odkaz:
http://arxiv.org/abs/0809.5151
Autor:
Siebert, A., collaboration, the RAVE
Publikováno v:
Astronomische Nachrichten; December 2008, Vol. 329 p892-895, 4p
