File:Eclipsing binary system in Orion.tif
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Size of this JPG preview of this TIF file: 684 × 599 pixels. Other resolutions: 274 × 240 pixels | 548 × 480 pixels | 728 × 638 pixels.
Original file (728 × 638 pixels, file size: 270 KB, MIME type: image/tiff)
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 02:01, 13 May 2020 | 728 × 638 (270 KB) | Acagastya | {{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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