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Classification and Identification of IRAS Sources with Low-Resolution Spectra IRAS low-resolution spectra were extracted for 11,224 IRAS sources.These spectra were classified into astrophysical classes, based on thepresence of emission and absorption features and on the shape of thecontinuum. Counterparts of these IRAS sources in existing optical andinfrared catalogs are identified, and their optical spectral types arelisted if they are known. The correlations between thephotospheric/optical and circumstellar/infrared classification arediscussed.
| Photoelectric photometry of M-type stars UBVRI photoelectric photometry was obtained for 110 M-type starscontained in the Caltech Two-Micron Survey and the revised AFGL Catalog.Of the 110 stars, 58 have a color index (B-R) greater than or equal to 4mag. A graph is given of (V-R) versus (V-I) for the present stars.
| The Distribution of the BD M-Type Stars Along the Galactic Equator. Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1958ApJ...128..510N&db_key=AST
| Bright Late M-Type Stars Near the Galactic Equator. Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1954ApJ...120..118N&db_key=AST
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Datos observacionales y astrométricos
Constelación: | Unicornio |
Ascensión Recta: | 06h24m46.94s |
Declinación: | +03°45'47.7" |
Magnitud Aparente: | 8.741 |
Movimiento Propio en Ascensión Recta: | -2.8 |
Movimiento Propio en Declinación: | -6.1 |
B-T magnitude: | 10.39 |
V-T magnitude: | 8.878 |
Catálogos y designaciones:
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