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- Hyades_Stream abstract "The Hyades Stream (or Hyades moving group) is a large collection of scattered stars that also share a similar trajectory with the Hyades Cluster. In 1869, Richard A. Proctor observed that numerous stars at large distances from the Hyades share a similar motion through space. In 1908, Lewis Boss reported almost 25 years of observations to support this premise, arguing for the existence of a co-moving group of stars that he called the Taurus Stream (now generally known as the Hyades Stream or following Eggen who assumed that it was a vestige of an initially more massive cluster which had partly evaporated, the Hyades Supercluster). Boss published a chart that traced the scattered stars' movements back to a common point of convergence.Eggen's argument that groups of this type are in fact cluster remnants has been debated. It has been noted that because such phenomena may also be the result of other dynamical mechanisms. Famaey B, et al. report that about 85% of stars in the Hyades Stream have been shown to be completely unrelated to the original cluster on the grounds of dissimilar age and metallicity; their common motion is attributed to tidal effects of the massive rotating bar at the center of the Milky Way Galaxy. Among the remaining members of the Hyades Stream, the exoplanet host star Iota Horologii has recently been proposed as an escaped member of the primordial Hyades Cluster.".
- Hyades_Stream wikiPageID "21978457".
- Hyades_Stream wikiPageLength "3060".
- Hyades_Stream wikiPageOutDegree "10".
- Hyades_Stream wikiPageRevisionID "602123933".
- Hyades_Stream wikiPageWikiLink Barred_spiral_galaxy.
- Hyades_Stream wikiPageWikiLink Category:Moving_groups.
- Hyades_Stream wikiPageWikiLink Exoplanet.
- Hyades_Stream wikiPageWikiLink Hyades_(star_cluster).
- Hyades_Stream wikiPageWikiLink Iota_Horologii.
- Hyades_Stream wikiPageWikiLink Lewis_Boss.
- Hyades_Stream wikiPageWikiLink Metallicity.
- Hyades_Stream wikiPageWikiLink Milky_Way.
- Hyades_Stream wikiPageWikiLink Moving_group.
- Hyades_Stream wikiPageWikiLink Richard_A._Proctor.
- Hyades_Stream wikiPageWikiLink Stellar_kinematics.
- Hyades_Stream wikiPageWikiLinkText "Hyades Stream".
- Hyades_Stream wikiPageWikiLinkText "Hyades moving group".
- Hyades_Stream hasPhotoCollection Hyades_Stream.
- Hyades_Stream wikiPageUsesTemplate Template:Reflist.
- Hyades_Stream subject Category:Moving_groups.
- Hyades_Stream hypernym Collection.
- Hyades_Stream type Book.
- Hyades_Stream type Group.
- Hyades_Stream type Association.
- Hyades_Stream type Group.
- Hyades_Stream comment "The Hyades Stream (or Hyades moving group) is a large collection of scattered stars that also share a similar trajectory with the Hyades Cluster. In 1869, Richard A. Proctor observed that numerous stars at large distances from the Hyades share a similar motion through space.".
- Hyades_Stream label "Hyades Stream".
- Hyades_Stream sameAs Corrente_delle_Iadi.
- Hyades_Stream sameAs Hyadengroep.
- Hyades_Stream sameAs m.05p2db7.
- Hyades_Stream sameAs Q1065564.
- Hyades_Stream sameAs Q1065564.
- Hyades_Stream sameAs 畢宿星流.
- Hyades_Stream wasDerivedFrom Hyades_Stream?oldid=602123933.
- Hyades_Stream isPrimaryTopicOf Hyades_Stream.