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The supermassive black hole in NGC4486a detected with SINFONI at the Very Large Telescope
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| The eclipsing binary system W CRU
Photoelectric UBV observations of W Cru were obtained between 1984 and1985 using the 50-cm Edith Winstone Blackwell Cassegrain telescope. Thelight curve presents a continuous 'Beta Lyrae'-like variation, alongwith peculier irregularities of the order of 0.1 mag. The possibility offitting both high-mass and low-mass models to the data is considered.
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Membro dei seguenti gruppi:
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Osservazione e dati astrometrici
| Costellazione: | Croce del Sud |
| Ascensione retta: | 12h12m10.90s |
| Declinazione: | -58°49'06.0" |
| Magnitudine apparente: | 8.53 |
| Distanza: | 231.481 parsec |
| Moto proprio RA: | -16.2 |
| Moto proprio Dec: | 2.7 |
| B-T magnitude: | 8.633 |
| V-T magnitude: | 8.539 |
Cataloghi e designazioni:
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