Abstract
We have analysed the data of 2.7 μm Equatorial Infrared Catalogue-1 (EIC-1) to study the space density distribution ofK andM type giants in the solar neighbourhood by attempting to fit the EIC-1 data with the models of Mikami and Ishida (1981) for space density distribution of late-type giants.
We present the results of our analysis.
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References
Elias, J. H.: 1978a,Astrophys. J. 233, 859.
Elias, J. H.: 1978b,Astrophys. J. 224, 453.
Johnson, H. L.: 1966,Ann. Rev. Astron. Astrophys. 4, 193.
Jones, T. J., Ashley, M., Hyland, A. R. and Ruelas-Mayorga, A.: 1981,Monthly Notices Roy. Astron. Soc. 197, 413.
Mikami, T. and Ishida, K.:Publ. Astron. Soc. Japan 33, 135 (MI).
Neugebauer, G. and Leighton, R. B.: 1969,Two-Micron Sky Survey NASA SP-3046 (TMSS).
Scargle, J. D. and Strecker, D. W.: 1979,Astrophys. J. 228, 838.
Sweeney, L. H., Heinsheimer, T. F., Yates, F. F., Maran, S. P., Lesh, J. R., and Nagy, T. A.: 1978,Interim Equatorial Infrared Catalogue, Number 1, Aerospace Report No. TR-0078 (3409-20)-1 (EIC-1).
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Ghosh, S.K., Tandon, S.N. The space density distribution of late-type giants in the solar neighbourhood. Astrophys Space Sci 87, 247–254 (1982). https://doi.org/10.1007/BF00648920
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DOI: https://doi.org/10.1007/BF00648920