The [Fe/H] Consistency of the Wolf 630 Moving Group

Details The [Fe/H] Consistency of the Wolf 630 Moving Group The [Fe/H] Consistency of the Wolf 630 Moving Group

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aas...185.4516t&link_type=abstract

American Astronomical Society, 185th AAS Meeting, #45.16; Bulletin of the American Astronomical Society, Vol. 26, p.1382

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The Wolf 630 moving group has been tested for [Fe/H] consistency by compiling data from [Fe/H] catalogs which include accidental errors. Catalog entries are available for 40 group stars; these stars make up 26% of the group members listed by Eggen in 1969. Three catalogs have been consulted (McWilliam 1990, ApJS, 74, 1075; Taylor 1991, ApJS, 76, 715; Taylor 1994, PASP, 106, 704). An F test shows that the group members are nonuniform in [Fe/H] at a confidence level exceeding 99.99%. The intrinsic +/- 2sigma scatter in [Fe/H] for the group members is found to be about 0.66 dex. Inspection of the data suggests that where metallicity is concerned, there is little to distinguish the Wolf 630 group from a random selection of nearby stars.

Affiliated with

Also associated with

No associations

Rating

The [Fe/H] Consistency of the Wolf 630 Moving Group 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 [Fe/H] Consistency of the Wolf 630 Moving Group, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The [Fe/H] Consistency of the Wolf 630 Moving Group will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1320793