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Parallaxes and Proper Motions of Prototypes of Astrophysically Interesting Classes of Stars

Published online by Cambridge University Press:  14 August 2015

V. Trimble
Affiliation:
1Physics Dept., Univ. of California, Irvine CA 92697 USA 2Astronomy Dept., Univ. of Maryland, College Park MD 207.12 USA
G.H. Herbig
Affiliation:
3Inst. for Astronomy, Univ. of Hawaii, Honolulu HI 96822 USA
A. Kundu
Affiliation:
2Astronomy Dept., Univ. of Maryland, College Park MD 207.12 USA 4Space Telescope Science Institute, Baltimore MD 21218

Extract

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Early release data were obtained under the 1982 announcement of opportunity for about two dozen stars belonging to seven classes whose basic properties or evolutionary status were uncertain at the time. A good many remain so. Many of the stars were too faint and far for parallaxes to be statistically significant, though many of the proper motions are. Two papers presenting the data have been accepted by archival journals (Trimble and Kundu 1997, 1998). Both bear the same title as this Abstract The first deals with the R Coronae Borealis variables, the second with the other six classes (FK Comae Stars, CVs, runaway T Tauri stars, and so forth).

Type
II. Joint Discussions
Copyright
Copyright © Kluwer 1998

References

Trimble, V. & Kundu, A. 1997. PASP (in press, October)Google Scholar
Trimble, V. & Kundu, A. 1998. AJ (in press, probably January)Google Scholar