The Vela Molecular Ridge is a prominent molecular cloud complex located in the southern hemisphere of the Milky Way galaxy, specifically in the constellation Vela. It is part of a larger region known for its dense concentrations of interstellar gas and dust, where star formation occurs. This area is characterized by its intricate structure, which includes dark filaments and regions of active star formation. The Vela Molecular Ridge is home to various interesting astronomical phenomena, including young star clusters and protostars.
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