Credit & Copyright: Yuexiao Shen,
Joe Hua
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.
1999 2000 2001 2002 2003 2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016 2017 2018 2019 2020 2021 2022 2023 2024 2025 |
Yanvar' Fevral' Mart Aprel' Mai Iyun' Iyul' Avgust Sentyabr' Oktyabr' Noyabr' Dekabr' |
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
|
Publikacii s klyuchevymi slovami:
molecular cloud - Molekulyarnye oblaka
Publikacii so slovami: molecular cloud - Molekulyarnye oblaka | |
Sm. takzhe:
Vse publikacii na tu zhe temu >> | |
