by APOD Robot » Thu Nov 23, 2023 5:06 am
Along the Taurus Molecular Cloud
Explanation: The cosmic brush of star formation composed
this interstellar canvas of emission, dust, and dark nebulae. A 5 degree wide telescopic mosaic, it frames a region found north of bright star Aldebaran on the sky, at an inner wall of
the local bubble along the
Taurus molecular cloud. At lower left, emission cataloged as
Sh2-239 shows signs of embedded young stellar objects. The region's Herbig-Haro objects, nebulosities associated with newly born stars, are marked by tell-tale reddish jets of shocked hydrogen gas. Above and right T Tauri, the prototype of the class of
T Tauri variable stars, is next to a yellowish nebula historically known as Hind's Variable Nebula (
NGC 1555). T Tauri stars are now generally recognized as young, less than a few million years old, sun-like stars still in the early
stages of formation.
[url=https://apod.nasa.gov/apod/ap231123.html] [img]https://apod.nasa.gov/apod/calendar/S_231123.jpg[/img] [size=150]Along the Taurus Molecular Cloud[/size][/url]
[b] Explanation: [/b] The cosmic brush of star formation composed [url=https://www.flickr.com/photos/150464529@N03/53336219347/]this interstellar canvas[/url] of emission, dust, and dark nebulae. A 5 degree wide telescopic mosaic, it frames a region found north of bright star Aldebaran on the sky, at an inner wall of [url=https://skyandtelescope.org/astronomy-news/1000-light-year-bubble-is-the-source-of-all-nearby-baby-stars/?utm_source=cc&utm_medium=newsletter]the local bubble[/url] along the [url=https://apod.nasa.gov/apod/ap111117.html]Taurus molecular cloud[/url]. At lower left, emission cataloged as [url=https://apod.nasa.gov/apod/ap111208.html]Sh2-239[/url] shows signs of embedded young stellar objects. The region's Herbig-Haro objects, nebulosities associated with newly born stars, are marked by tell-tale reddish jets of shocked hydrogen gas. Above and right T Tauri, the prototype of the class of [url=https://www.aavso.org/vsots_ttau]T Tauri variable stars[/url], is next to a yellowish nebula historically known as Hind's Variable Nebula ([url=https://apod.nasa.gov/apod/ap220210.html]NGC 1555[/url]). T Tauri stars are now generally recognized as young, less than a few million years old, sun-like stars still in the early [url=https://universe.nasa.gov/stars/basics/]stages of formation[/url].
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