File:Brightness dip and velocity variations of OGLE-TR-122.tif

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English: The top panel shows the brightness dip of OGLE-TR-122 as measured by OGLE. The signal from the star is reduced by 1.5% for a little more than 3 hours. This is the probable indication that an object passed in front of the star. The bottom panel presents the velocity variations of the star. They were determined with the FLAMES instrument on the VLT. The orbital solution fitting the data is also shown as the solid line. These measurements indicate the presence of a low-mass stellar companion to OGLE-TR-122.
Date 3 March 2005
Source https://www.eso.org/public/images/eso0507a/
Author ESO
Other versions JPEG: File:Brightness «Dip» and Velocity Variations of OGLE-TR-122.jpg

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Date/TimeThumbnailDimensionsUserComment
current18:27, 25 June 2023Thumbnail for version as of 18:27, 25 June 20231,571 × 1,495 (148 KB)Юрий Д.К. (talk | contribs)Uploaded a work by ESO from https://www.eso.org/public/images/eso0507a/ with UploadWizard

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