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Can physical stellar collisions explain the blue stragglers in the dwarf spheroidal galaxies?

Conference ·
OSTI ID:10136322

The hypothesis that the blue stragglers in the dwarf spheroidal galaxie have a collisional origin is considered. If all of the dark matter in these galaxies is in the form of low-mass stars and the binary frequency is {approx_equal} 50%, then it is quite possible that {approx_equal} 10% to 20% of their blue stragglers have been produced by physical stellar collisions.

Research Organization:
Los Alamos National Lab., NM (United States)
Sponsoring Organization:
USDOE, Washington, DC (United States)
DOE Contract Number:
W-7405-ENG-36
OSTI ID:
10136322
Report Number(s):
LA-UR--93-467; CONF-9210324--1; ON: DE93008711
Country of Publication:
United States
Language:
English

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