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ICCD Speckle Observations of Binary Stars.XV.An Investigation of Lunar Occultation Systems
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1996AJ....112.2260M&db_key=AST
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| Supplement to the Second Catalogue of Am Stars with Known Spectral Types (end 1981)
Not Available
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Classifications are given for 865 components of visual multiples; theyshow no systematic differences from the MK system, and the random errorsare one subclass in type and two-thirds of a luminosity class. It isfound that at least 1% of the F-type IV and V stars are weak-lined, 32%of the A4-F1 IV and V stars are Am, and 5% of the A0-A3 IV and V starsare early-type Am. Attention is called to the large fraction (55%) ofthe A3-A9 III-V stars that are of luminosity classes III or IV, unlikethe percentage (16%) at neighboring types.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Taurus |
| Ascensió Recta: | 04h08m20.64s |
| Declinació: | +19°44'15.5" |
| Magnitud Aparent: | 7.744 |
| Distancia: | 279.33 parsecs |
| Moviment propi RA: | -2 |
| Moviment propi Dec: | -6.2 |
| B-T magnitude: | 8.076 |
| V-T magnitude: | 7.772 |
Catàlegs i designacions:
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