Explanation: Centered in this colorful cosmic canvas, NGC 2626 is a beautiful, bright, blue reflection nebula in the southern Milky Way. Next to an obscuring dust cloud and surrounded by reddish hydrogen emission from large H II region RCW 27 it lies within a complex of dusty molecular clouds known as the Vela Molecular Ridge. NGC 2626 is itself a cloud of interstellar dust reflecting blue light from the young hot embedded star visible within the nebula. But astronomical explorations reveal many other young stars and associated nebulae in the star-forming region. NGC 2626 is about 3,200 light-years away. At that distance this telescopic field of view would span about 30 light-years along the Vela Molecular Ridge.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
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: reflection nebula - molecular cloud - otrazhatel'nye tumannosti - Molekulyarnye oblaka Publikacii so slovami: reflection nebula - molecular cloud - otrazhatel'nye tumannosti - Molekulyarnye oblaka
Sm. takzhe: Otrazheniya v vdB 31 Peremennaya tumannost' NGC 2261 Zvezdnaya pyl' v molekulyarnom oblake Perseya IC 348 i Barnard 3 Ruka pomoshi v Kassiopee Prizraki v Kassiopee NGC 6727: tumannost' Buinyi Pavian Vse publikacii na tu zhe temu >>