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Speckle Interferometry at the US Naval Observatory. VIII.
The results of 2044 speckle interferometric observations of doublestars, made with the 26 inch (66 cm) refractor of the US NavalObservatory, are presented. Each speckle interferometric observation ofa system represents a combination of over a thousand short-exposureimages. These observations are averaged into 1399 mean positions andrange in separation from 0.16" to 14.97", with a mean separation of2.51". This is the eighth in a series of papers presenting measuresobtained with this system and covers the period 2001 March 18 through2001 December 30.
| Mesures d'etoiles doubles faites a Nice.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1978A&AS...33..275M&db_key=AST
| The visual magnitudes of double stars.
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Observation and Astrometry data
| Constellation: | Persée |
| Right ascension: | 02h46m21.19s |
| Declination: | +53°09'46.7" |
| Apparent magnitude: | 8.276 |
| Distance: | 10000000 parsecs |
| Proper motion RA: | -1.9 |
| Proper motion Dec: | -4.9 |
| B-T magnitude: | 10.605 |
| V-T magnitude: | 8.469 |
Catalogs and designations:
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