Free Newsletters - Space - Defense - Environment - Energy - Solar - Nuclear
by Staff Writers
Munich, Germany (SPX) Feb 11, 2013
Running along the border between the constellations of Canis Major (The Great Dog) and Monoceros (The Unicorn) in the southern sky, the Seagull Nebula is a huge cloud mostly made of hydrogen gas. It's an example of what astronomers refer to as an HII region. Hot new stars form within these clouds and their intense ultraviolet radiation causes the surrounding gas to glow brightly.
The reddish hue in this image is a telltale sign of the presence of ionised hydrogen . The Seagull Nebula, known more formally as IC 2177, is a complex object with a bird-like shape that is made up of three large clouds of gas - Sharpless 2-292 (eso1237) forms the "head", this new image shows part of Sharpless 2-296, which comprises the large "wings", and Sharpless 2-297 is a small, knotty addition to the tip of the gull's right "wing" .
These objects are all entries in the Sharpless nebula catalogue, a list of over 300 glowing clouds of gas compiled by American astronomer Stewart Sharpless in the 1950s. Before he published this catalogue Sharpless was a graduate student at the Yerkes Observatory near Chicago, USA, where he and his colleagues published observational work that helped to show that the Milky Way is a spiral galaxy with vast, curved arms.
Spiral galaxies can contain thousands of HII regions, almost all of which are concentrated along their spiral arms. The Seagull Nebula lies in one of the spiral arms of the Milky Way. But this is not the case for all galaxies; while irregular galaxies do contain HII regions, these are jumbled up throughout the galaxy, and elliptical galaxies are different yet again - appearing to lack these regions altogether. The presence of HII regions indicates that active star formation is still in progress in a galaxy.
This image of Sharpless 2-296 was captured by the Wide Field Imager (WFI), a large camera mounted on the MPG/ESO 2.2-metre telescope at ESO's La Silla Observatory in Chile. It shows only a small section of the nebula, a large cloud that is furiously forming hot stars in its interior. The frame shows Sharpless 2-296 lit up by several particularly bright young stars - there are many other stars scattered across the region, including one so bright that stands out as the gull's "eye" in pictures of the entire complex.
Wide-field images of this region of the sky show a multitude of interesting astronomical objects. The young bright stars within the nebula are part of the nearby star-forming region of CMa R1 in the constellation of Canis Major, which is filled with bright stars and clusters.
Notes:  Astronomers use the term HII to mean ionised hydrogen and HI for atomic hydrogen. A hydrogen atom consists of an electron bound to a proton but in an ionised gas atoms are split into freely moving electrons and positive ions, in this case just single protons.  These objects are officially designated Sh 2-292, Sh 2-296, and Sh 2-297 respectively in the SIMBAD astronomical database.
Stellar Chemistry, The Universe And All Within It
|The content herein, unless otherwise known to be public domain, are Copyright 1995-2014 - Space Media Network. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA Portal Reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. Advertising does not imply endorsement,agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. Privacy Statement|