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The kinematics of the Small Magellanic Cloud from its field carbon stars

Journal Article · · Astrophysical Journal; (USA)
DOI:https://doi.org/10.1086/167790· OSTI ID:5288347
; ;  [1]
  1. Observatoire du Mont Megantic, Sainte-Foy (Canada)
The present velocity survey observed 150 carbon stars in the SMC in the near-IR with an individual precision of + or - 1.8 km/sec. Carbon stars are found to behave kinematically like the planetary nebulae system with which they share a velocity dispersion of about 27 km/sec; they also exhibit the same velocity dispersion as a sample of halo metal-poor giants near NGC 121. The carbon stars and planetary nebulae may belong to a spheroidal system, and indications are found of streaming motions in the wing section between the SMC and LMC. 26 refs.
OSTI ID:
5288347
Journal Information:
Astrophysical Journal; (USA), Journal Name: Astrophysical Journal; (USA) Vol. 344; ISSN ASJOA; ISSN 0004-637X
Country of Publication:
United States
Language:
English

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