The binary frequency of the OBN and OBC stars

Details The binary frequency of the OBN and OBC stars The binary frequency of the OBN and OBC stars

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...222..234b&link_type=abstract

Astrophysical Journal, Part 1, vol. 222, May 15, 1978, p. 234-245. Research supported by the National Research Council of Canad

Astronomy and Astrophysics

Astrophysics

62

Abundance, Atomic Spectra, Binary Stars, Line Spectra, Stellar Spectra, Boron, Carbon, Nitrogen, Oxygen Spectra, Periodic Variations, Tables (Data)

Scientific paper

Radial velocity measurements for a class of early-type stars having either enhanced carbon or nitrogen line strengths (termed OBCN stars) are undertaken to evaluate the binary frequency of the OBN and OBC subgroups. Between 50 and 100% of the OBN stars appear to be short-period binaries, while none of the OBC stars fall into this category. Mass-transfer evolution in binary systems may thus offer a reasonable explanation for the abundance anomalies exhibited by the OBN stars. The possibility that the OBN and OBC stars are kinematically distinct subgroups is also discussed.

Affiliated with

Also associated with

No associations

Rating

The binary frequency of the OBN and OBC stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The binary frequency of the OBN and OBC stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The binary frequency of the OBN and OBC stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1296044