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The HST's view of M81, with its open star clusters, globular star clusters, and regions of fluorescent gas.
The HST's view of M81, with its open star clusters, globular star clusters, and regions of fluorescent gas.
An infrared image of Messier 81 taken by the Spitzer Space Telescope. The blue colors represent stellar emission observed at 3.6 μm. The green colors
An infrared image of Messier 81 taken by the Spitzer Space Telescope. The blue colors represent stellar emission observed at 3.6 μm. The green colors represent 8 μm emission originating primarily from polycyclic aromatic hydrocarbons in the interstellar medium. The red colors represent 24 μm emission originating from heated dust in the interstellar medium.
M81 (left) and M82 (right). M82 is one of two galaxies strongly influenced gravitationally by M81. The other, NGC 3077, is located off the top edge of
M81 (left) and M82 (right). M82 is one of two galaxies strongly influenced gravitationally by M81. The other, NGC 3077, is located off the top edge of this image.
M81 with satellite galaxy Holmberg IX, shown top center-right.
M81 with satellite galaxy Holmberg IX, shown top center-right.
Nova
Artist's conception of a white dwarf, right, accreting hydrogen from the Roche lobe of its larger companion star
Artist's conception of a white dwarf, right, accreting hydrogen from the Roche lobe of its larger companion star
Nova Eridani 2009 (apparent magnitude ~8.4)
Nova Eridani 2009 (apparent magnitude ~8.4)
GK Persei: Nova of 1901
GK Persei: Nova of 1901
Nova in Andromeda Galaxy
Nova in Andromeda Galaxy