TW Horologii and NGC 1252 - A rebuttal

Details TW Horologii and NGC 1252 - A rebuttal TW Horologii and NGC 1252 - A rebuttal

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pasp...96...70e&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 96, Jan. 1984, p. 70, 71.

Astronomy and Astrophysics

Astronomy

3

Carbon Stars, Star Clusters, Variable Stars, Astronomical Photometry, Open Clusters, Stellar Motions

Scientific paper

The Bouchet and The(1983) suggestion that the carbon variable TW Hor is a member of the open cluster NGC 1252 is questioned on the basis of Cape Zone Catalog data for the ten stars observed by them. The most probable membership for the variable is presently held to be in the Hyades Supercluster, and a distance modulus of 7.7 mag is given. Bouchet and The's derived distance of 500 parsecs would place NGC 1252 400 pc above the galactic plane, which is higher than might be expected for what they regard as a young disk cluster.

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