The Rosette Nebula (aka NGC 2237) comes with a long stem of glowing hydrogen gas. At the edge of a large molecular cloud in Monoceros, some 5,000 light years away, the petals of this rose are actually a stellar nursery whose lovely, symmetric shape is sculpted by the winds and radiation from its central cluster of hot young stars.
Clouds of Perseus ~ contains over 10,000 solar masses of gas and dust, but the eye is drawn to red NGC 1499. Known as the California Nebula, its characteristic glow of atomic hydrogen gas is fueled by ultraviolet light from luminous blue star Xi Persei. Farther along, intriguing young star cluster IC 348 and neighboring Flying Ghost Nebula. On the outskirts of a giant molecular cloud, another active star forming region, NGC 1333, lies near the edge of the wide field of view.