Matches in DBpedia 2016-04 for { ?s ?p "HD 895 is a triple star system in the constellation Andromeda. Its apparent magnitude is 6.27. Located around 131 parsecs (430 ly) away, the primary is a F-type main-sequence star of spectral type F8V, a star that is currently fusing its core hydrogen. While the secondary star cannot be separated from the primary except by spectroscopy, the tertiary can, and has been found to be a spectroscopic binary itself, although with an apparent magnitude of 10.37, it is too faint to be seen without a telescope."@en }
Showing triples 1 to 2 of
2
with 100 triples per page.
- HD_895 abstract "HD 895 is a triple star system in the constellation Andromeda. Its apparent magnitude is 6.27. Located around 131 parsecs (430 ly) away, the primary is a F-type main-sequence star of spectral type F8V, a star that is currently fusing its core hydrogen. While the secondary star cannot be separated from the primary except by spectroscopy, the tertiary can, and has been found to be a spectroscopic binary itself, although with an apparent magnitude of 10.37, it is too faint to be seen without a telescope.".
- Q1748091 abstract "HD 895 is a triple star system in the constellation Andromeda. Its apparent magnitude is 6.27. Located around 131 parsecs (430 ly) away, the primary is a F-type main-sequence star of spectral type F8V, a star that is currently fusing its core hydrogen. While the secondary star cannot be separated from the primary except by spectroscopy, the tertiary can, and has been found to be a spectroscopic binary itself, although with an apparent magnitude of 10.37, it is too faint to be seen without a telescope.".