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English: The shell of V5668 Sgr imaged at 230 GHz with the ALMA array. The image has been convolved with a gaussian function to make it match the resolution of the Hubble Space Telescope at the wavelength of H-alpha. The major tick marks are separated by 100 mas. The image is monochromatic; the colors represent intensity. This image was taken from Diaz et al. 2018, MNRAS Letters, Vol 480, issue 1, L54-L57 (doi 10.1093/mnrasl/sly121). Uploaded with the permission of the paper's first author.
Date
Source Diaz et al. 2018, MNRAS Vol 480, issue 1, pp L54-L57
Author PopePompus

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10 January 2021

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Date/TimeThumbnailDimensionsUserComment
current22:26, 10 January 2021Thumbnail for version as of 22:26, 10 January 2021869 × 868 (319 KB)PopePompusRemoved beam circle and added indication of image orientation
21:53, 10 January 2021Thumbnail for version as of 21:53, 10 January 2021869 × 868 (398 KB)PopePompusCross-wiki upload from en.wiki.x.io

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