star formation tagged posts

The Spider Nebula lies about 10,000 light-years away from Earth and is a site of active star formation. Infrared wavelengths have been assigned visible colors. Light with a wavelength of 1.2 microns, detected by 2MASS, is shown in blue. The Spitzer wavelengths of 3.6 and 4.5 microns are green and red, respectively. Credit: NASA/JPL-Caltech/2MASS

A nebula known as “the Spider” glows fluorescent green in an infrared image from NASA’s Spitzer Space Telescope and the Two Micron All Sky Survey (2MASS). The Spider, officially named IC 417, lies near a much smaller object NGC 1931. Together, the two are called “The Spider and the Fly” nebulae. Nebulae are clouds of interstellar gas and dust where stars can form.

The Spider, ~10,000 light-years from Earth in the constellation Auriga, is clearly a ...

Credit: ESA/Hubble and NASA; Acknowledgement: Judy Schmidt

Despite being less famous than their elliptical and spiral galactic cousins, irregular dwarf galaxies, such as the one captured in this NASA/ESA Hubble Space Telescope image, are actually one of the most common types of galaxy in the universe. Known as UGC 4459, this dwarf galaxy is located 11 million light-years away in constellation of Ursa Major (The Great Bear), a constellation that is also home to the Pinwheel Galaxy (M101), the Owl Nebula (M97), Messier 81, Messier 82 and several other galaxies all part of the M81 group.

UGC 4459’s diffused and disorganized appearance is characteristic of an irregular dwarf galaxy...

Animated map of Orion’s Horsehead Nebula showing 100 separate views in sequence. The yellow and white areas have the most intense radiation from carbon atoms. Credits: NASA/DLR/USRA/DSI/SOFIA/GREAT Consortium

NASA’s Stratospheric Observatory for Infrared Astronomy, or SOFIA, has released a new map of the interstellar cloud called the Horsehead Nebula, in constellation Orion. This map is made of 100 separate views of the nebula, each mapping carbon atoms at different velocities. When combined, these different views create a multi-faceted representation of the nebula. Each location on this new SOFIA map of the nebula contains a far-infrared spectrum of the gas and dust there, allowing astronomers to examine the dynamics, chemistry, temperatures, and velocity within the nebula...

In an artist’s conception, heated galactic wind shown in the hazy portion of the picture emanates from the bright quasar at the edge of a black hole, scattering dust and gas. If allowed to cool and condense, that dust and gas would instead begin to form stars. Credit: Johns Hopkins University

Quasars slowed star formation new research shows. It appears intense radiation and galaxy-scale winds emitted by the quasars – the most luminous objects in the universe – heats up clouds of dust and gas. The heat prevents that material from cooling and forming more dense clouds, and eventually stars.

They looked at information on 17,468 galaxies and found a tracer of energy called the Sunyaev-Zel’dovich Effect...