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HD 56525


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An IRAS survey of main sequence B, A, and F stars
Results are presented of an IRAS survey of main-sequence B, A, and Fstars, based on three primary sources as a data base: theBernacca-Perinotto Catalog of Stellar Rotational Velocities, theMichigan Spectral Catalog, and the Bright Star Catalog. The stars in thedata base are divided into four categories: (1) main-sequence singlestars, (2) main-sequence close binary stars, (3) spectrally peculiarstars such as Am, Ap, Fm, and Fp stars, and (4) subgiants. It is foundthat about 20 percent of main-sequence single stars show an IR colorexcess in at least one of the 12, 25, or 60 micron IRAS bands, while theother three groups do not show any statistically significant percentageof IR color excess stars. It is also found that stars with large (v sini) values are more likely to show color excesses at IRAS wavelengthsthan stars with small (v sin i) values.

Investigation of a Milky Way field in Canis Major
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1974AJ.....79.1022C&db_key=AST

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Observation and Astrometry data

Constellation:Grand Chien
Right ascension:07h16m47.06s
Declination:-13°40'52.0"
Apparent magnitude:7.18
Distance:269.542 parsecs
Proper motion RA:-3.1
Proper motion Dec:-1.4
B-T magnitude:7.266
V-T magnitude:7.188

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 56525
TYCHO-2 2000TYC 5407-2485-1
USNO-A2.0USNO-A2 0750-03822881
HIPHIP 35220

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