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Multichannel astrometric photometer parallax studies in the regions of Groombridge 1618, Zeta Bootis, and Sigma Draconis
Improved trigonometric parallaxes are reported for stars in the regionsof Groombridge 1618, Zeta Bootis, and Sigma Draconis which differ fromgenerally accepted parallaxes by two to five standard deviations. Theweighted mean parallax of Groombridge 1618 becomes 0.2079 +/- 0.0013arcsec, indicating a distance modulus of -1.59 +/- 0.014 and yielding anabsolute magnitude of this K7 V star of 8.20 +/- 0.017. The parallaxdetermined for the visual binary Zeta Bootis is 0.0202 +/- 0.0010 arcsecand implies an average absolute visual magnitude of 1.067 +/- 0.12 forthe spectroscopically similar components. The weighted mean parallax ofSigma Draconis becomes 0.1747 +/- 0.0010 arcsec, indicating a distancemodulus of -1.210 +/- 0.012 and yielding an absolute visual magnitude of5.90 +/- 0.012 for this K0 V star. The absolute visual magnitudes of thehigh velocity star Roman 336 and of the subdwarf star AO 1187 are foundto be + 4.0 +/- 0.13 and + 5.9 +/- 0.17, respectively.
| Photometry of astrometric reference stars
UBVRI, DDO, and uvby, H-beta photometry of astrometric reference starsis presented. Spectral types and luminosity classifications made fromthe colors are used to determine their spectroscopic parallaxes. In thispaper, colors for 309 stars in 25 regions are given, and classificationsfor 210 stars have been made. These stars form reference frames in theAllegheny Observatory Multichannel Astrometric Photometer astrometricprogram, and in the Praesepe cluster reduced by Russell (1976). It isfound that the present photometric spectral types are reliable to within2.5 spectral subclasses.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Bootes |
| Ascensió Recta: | 14h40m10.56s |
| Declinació: | +13°51'24.4" |
| Magnitud Aparent: | 9.123 |
| Moviment propi RA: | -61.5 |
| Moviment propi Dec: | -6.9 |
| B-T magnitude: | 10.285 |
| V-T magnitude: | 9.219 |
Catàlegs i designacions:
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