The brightest stars and the distance to the dwarf galaxy HO IX

Details The brightest stars and the distance to the dwarf galaxy HO IX The brightest stars and the distance to the dwarf galaxy HO IX

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26as...89..529g&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 89, no. 3, Sept. 1991, p. 529-536.

Astronomy and Astrophysics

Astrophysics

26

Astronomical Photometry, Color-Magnitude Diagram, Dwarf Galaxies, Stellar Luminosity, Stellar Magnitude, Blue Stars, Charge Coupled Devices, Supergiant Stars, Telescopes

Scientific paper

The magnitudes and colors of the brightest stars in the area of Ho IX were determined from photometric data extracted from the B and V plates obtained with a 6-m telescope. A comparison of the results with data of Sandage (1984), Davidge and Jones (1989), and Hopp and Schulte-Ladbeck (1987) disclosed systematic discrepancies between new and published data. The new color-magnitude diagram was used to select the brightest supergiants. For three red stars and three blue stars of this group, the average values were found to be V(3R) = 19.96 mag and B(3B) = 20.66 mag, respectively.

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