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Sodium enrichment of stellar atmospheres. I. Non-variable supergiants and bright giants 48 supergiants and bright giants have been observed in order toinvestigate the sodium enrichment of their atmospheres and itsconnection with stellar gravity. We present the equivalent widths of the6154 Å and 6160 Å Na I lines measured from the programspectra, the results of effective temperature determinations, the NLTEsodium abundances, and the derived relation between the sodiumoverabundance and surface gravity.
| A photometric study of wide visual double stars. II - Common proper motion double stars A total of 82 common proper motion wide visual double stars have beenobserved using the uvby, H-beta systems. MK class, color excess,absolute magnitude, effective temperature, and distance have beenderived from calibrations of the above systems. From the distancesderived here and the astrometric data, taken from the literature, it wasfound that the percentage of physical binaries among the common propermotion wide double stars is significantly higher than the samepercentage among the wide visual double stars with significant relativeproper motion, but there are a lot of optical pairs among them as well.
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| Relationship between CN anomaly and U V W components of space velocity. Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1962AJ.....67..757Y&db_key=AST
| 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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Osservazione e dati astrometrici
Costellazione: | Pegaso |
Ascensione retta: | 22h14m48.57s |
Declinazione: | +22°31'24.3" |
Magnitudine apparente: | 6.635 |
Distanza: | 277.778 parsec |
Moto proprio RA: | 3.6 |
Moto proprio Dec: | -9.2 |
B-T magnitude: | 7.797 |
V-T magnitude: | 6.731 |
Cataloghi e designazioni:
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