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LDN 1641

LDN 1641 or Lynds 1641 is a dark cloud in the constellation Orion. It encompasses a large part of the Orion A molecular cloud in the Orion molecular cloud complex, which is the closest giant molecular cloud to earth. At its northern end it is connected to the Orion Nebula and at its southern end it is connected to the dark cloud LDN 1647. LDN 1641 contains more than a thousand young stellar objects (YSOs). It is a relative low density star-forming region without any massive O- or B-type stars that could disturb the formation of young stars with their ultraviolet radiation. This means that researchers can study star formation that is happening in a very different environment when compared to the Orion Nebula.

Gallery
File:Euclid peers through a dark cloud’s dusty veil ESA514088.jpg|LDN 1641 imaged by the Euclid Space Telescope|alt=The focus of the image is a portion of LDN 1641, an interstellar nebula in the constellation of Orion. In this view, a deep-black background is sprinkled with a multitude of dots (stars) of different sizes and shades of bright white. Across the sea of stars, a web of fuzzy tendrils and ribbons in varying shades of orange and brown rises from the bottom of the image towards the top-right like thin coils of smoke. File:Wide-field view of part of Orion nebula in visible light.jpg|Orion Nebula (top bright cloud) and Lynds 1641 (bottom dark clouds) with the Digitized Sky Survey 2 File:Nrao20in02 herschellayout NoLabels02062020-scaled.jpg|Orion A (bottom) with Herschel. Yellow points of the bottom cloud show the position of young stellar objects in Lynds 1641. The bottom three disks are in Lynds 1641. File:Sword of Orion, Orion nebula - Herschel - Nhsc2016-003b.tif|Herschel Space Observatory image of Lynds 1641 (orange) and the Orion Nebula (middle circle, white) and Sh2-279 (top circle, white). == References ==
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