The nebulae is more or
less solid, evident or not from Earth. Nebulae can be found anywhere in the
interstellar space. Before the invention of the telescope, the term nebula was
applied to all celestial objects of diffuse appearance. As a result, many
objects are now known to be star clusters of galaxies were called nebulae. Nebulae
have been detected in almost all galaxies, including our own, the Milky Way.
Depending on the age of stars associated, it can be classified into two groups:
1. - Associated evolved stars, such as planetary nebulae and supernova
remnants. 2. - Associated with very young stars, some even still in the process
of training, such as Herbig-Haro objects and molecular clouds.
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Monday, June 11, 2012
Star clusters
Star cluster is a group of stars detained jointly
since regards the result of gravitation. Star clusters are classified into two
groups: open clusters, which have no definite shape, and globular clusters,
which are spherical or nearly spherical. The open consist of a few hundred
young stars, while globular clusters contain more than a thousand times that
amount, and are generally very old stars. Globular clusters form a halo around
our galaxy, the Milky Way, while the open is located in the spiral arms. Open
clusters are much more numerous than globular: about 1,000 are known in our
galaxy and there are only 140 globular.
What is the Milky Way?

Instinctive hub four arms: Arm Peruses, Orion Arm,
Arm Cross Arm Sagittarius and Centaurs. Form a slowly rotating disk in a
spiral. In the arms are the youngest stars, White and Blue. There are also many
nebulae where new stars form. The Sagittarius Arm is the brightest of all.
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