File:Eclipsing binary system in Orion.tif
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DescriptionEclipsing binary system in Orion.tif |
English: The RXJ 0529.4+0041 system after secondary eclipse. The object RXJ 0529.4+0041 was first discovered by the X-ray satellite ROSAT. Subsequent optical spectroscopy showed this object to be a young, low-mass spectroscopic binary system. And when a team of astronomers used a 91-cm telescope at the Serra La Nave observing station on the slope of the Etna volcano (Sicily) to monitor the light curve, they also discovered that this system undergoes eclipses.
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Date | |
Source | European Southern Observatory |
Author | ESO |
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current | 02:01, 13 May 2020 | 728 × 638 (270 KB) | Acagastya (talk | contribs) | {{Information |description ={{en|1=The RXJ 0529.4+0041 system after secondary eclipse. The object RXJ 0529.4+0041 was first discovered by the X-ray satellite ROSAT. Subsequent optical spectroscopy showed this object to be a young, low-mass spectroscopic binary system. And when a team of astronomers used a 91-cm telescope at the Serra La Nave observing station on the slope of the Etna volcano (Sicily) to monitor the light curve, they also discovered that this system undergoes eclipses. Thi... |
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File change date and time | 11:44, 20 January 2009 |
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