Blue stragglers

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Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pasp..105.1081s&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 105, no. 692, p. 1081-1100

Astronomy and Astrophysics

Astronomy

104

Binary Stars, Blue Stars, Color-Magnitude Diagram, Star Clusters, Stellar Evolution, Dwarf Galaxies, Mass Transfer, Metallicity, Mixing, Stellar Magnetic Fields, Stellar Rotation

Scientific paper

It is becoming clearer that several mechanisms, difficult to distinguish, must be responsible for the blue-straggler phenomenon. It is also highly that more than one mechanism occurs even within the same cluster to produce blue-straggler stars (BSs). There is still some ambiguity about whether BSs are single or double stars, simply because of the possibility that some BSs have merged. In the youngest clusters, perhaps high rotation in single BSs provide support for internal mixing; BSs in young to intermediate-age clusters are likely to receive this mixing support from high magnetic fields; in old-disk open clusters, globulars, and perhaps dwarf galaxies, binary mass transfer, and binary merger are likely the major causes for the production of BSs, with a contribution from binary-binary collisions and coalescence. There is considerable observational evidence of the existence of binaries in these systems. Progress has been certainly made in the last 40 yr, but BSs remain an intriguing challenge.

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