Narrow-band photometry of late-type stars. II

Details Narrow-band photometry of late-type stars. II Narrow-band photometry of late-type stars. II

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...68..259h&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 68, no. 2, March 1987, p. 259-282.

Astronomy and Astrophysics

Astrophysics

19

Late Stars, Solar Neighborhood, Star Distribution, Stellar Spectrophotometry, Ubv Spectra, Galactic Structure, Narrowband, Star Clusters

Scientific paper

This paper presents extensive narrow-band photometry in the Uppsala system supplementing earlier published mesurements so that data now are available for all late-type stars brighter than V = 6.05 and a number of galactic cluster members. Numerous UBV and BV measurements are also published. The data are used to determine relations for the prediction of UBV intrinsic colors for late-type stars from the narrow-band measurements. The main purpose of the data is to constitute the basis for the determination of solar-neighborhood space densities of late-type stars, mainly giants of different kinds; these space densities will be combined with narrow-band data for fainter stars in the north Galactic pole region to yield the decrease of space density with distance from the galactic plane for many kinds of late-type stars.

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