File:J1407b ALMA Kenworthy et al. 2020 Fig1.jpg

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English: ALMA image of the field towards J1407. The location of the star J1407 in 2017 is shown as a white square, and the white triangle gives the location at the time of the eclipse in 2007. The white ring indicates the expected location for an object travelling at 35 km s−1 between the two epochs (assuming that the object is co-distant with J1407); the dotted lines represent the 1σ uncertainties. The detected ALMA source is at a position angle of approximately 95 degrees. The ALMA beam is shown in the lower left corner.
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Source Figure 1 from https://doi.org/10.1051/0004-6361/201936141
Author M. A. Kenworthy et al./ALMA/ESO/AUI/NRAO/NAOJ/NSF, published by Astronomy & Astrophysics/EDP Sciences

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current19:25, 8 July 2024Thumbnail for version as of 19:25, 8 July 20241,200 × 897 (608 KB)Nrco0e (talk | contribs)Uploaded a work by M. A. Kenworthy et al./ALMA/ESO/AUI/NRAO/NAOJ/NSF, published by Astronomy & Astrophysics/EDP Sciences from [https://www.aanda.org/articles/aa/full_html/2020/01/aa36141-19/F1.html Figure 1] from https://doi.org/10.1051/0004-6361/201936141 with UploadWizard

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