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Speckle Observations of Binary Stars with the WIYN Telescope. III. A Partial Survey of A, F, and G Dwarfs
Two hundred thirty nearby main-sequence stars with spectral types in therange of A to G have been observed by way of speckle interferometryusing the WIYN 3.5 m telescope at Kitt Peak, Arizona. The stars had noprevious mention of duplicity in the literature. Of those observed, 14showed clear evidence of a companion, and 63 were classified assuspected nonsingle based on a power spectrum analysis. The remainingstars discussed show no evidence of duplicity to the limit of thedetection system in high-quality observations. The WIYN Observatory is ajoint facility of the University of Wisconsin-Madison, IndianaUniversity, Yale University, and the National Optical AstronomyObservatory.

Spectral and Luminosity Classifications and Measurements of the Strength of Cyanogen Absorption for Late-Type Stars from Objective-Prism Spectra.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1961ApJ...134..809Y&db_key=AST

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Dades d'Observació i Astrometria

Constel·lació:Ursa Major
Ascensió Recta:09h53m57.96s
Declinació:+57°41'01.3"
Magnitud Aparent:7.458
Distancia:79.872 parsecs
Moviment propi RA:36.9
Moviment propi Dec:-92.7
B-T magnitude:8.443
V-T magnitude:7.54

Catàlegs i designacions:
Noms Propis   (Edit)
HD 1989HD 85472
TYCHO-2 2000TYC 3820-864-1
USNO-A2.0USNO-A2 1425-07406383
HIPHIP 48537
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