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File:Proplyd Lambda Orionis.png

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Description
English: Dusty proplyds in the star cluster Collinder 69 (Lambda Orionis Cluster), which appears as a star leaving a red tail behind. The external evaporation of dust from the disk of this object is caused by nearby OB-stars. The dust is then swept away by the nearby OB-star Meissa (Lambda Orionis), forming a tail in the wake of the young stars.

The two boxed areas had separate image processing for the red channel.

Image Credit: NASA Spitzer Space Telescope

Filters: 4.5, 8.0 and 24 Micron
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Source Own work
Author Meli thev

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15 May 2023

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current17:43, 15 May 2023Thumbnail for version as of 17:43, 15 May 2023878 × 909 (469 KB)Meli thevUploaded own work with UploadWizard

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