or vote for the best nickname!
(To vote for a nickname, first search the for nickname & then click the vote button beside it.)
You can also add comments on nicknames
such as meaning or a short profile.
Comments
Googlism comments
supernovae is barely visible in the k
supernovae is not new
supernovae is needed either to yield a value for the density of
supernovae is needed either to yield a value for the
supernovae is for supernovae at a distance of 100
supernovae is probably not constant over the age of the galaxy
supernovae is different
supernovae is created when a binary star system consisting of a red giant and a white dwarf exchange mass
supernovae is based on particle oscillations
supernovae is a kind of astrophysical objects whose radiation covers the whole band from radio to rays
supernovae is observable fact
supernovae is important because of the need to get vital spectroscopic information for type classification while the system is still
supernovae is far more infrequent an event than a brilliant comet
supernovae is one of the major scientific objectives of integral
supernovae is along the carina galactic arm
supernovae is a huge
supernovae is a very active field of astronomy
supernovae is 984
supernovae is patchy
supernovae is relatively unexplored
supernovae is nothing short of serendipitous
supernovae is the same as the one deduced from nearby ones
supernovae is polarized that is
supernovae is constantly being updated with space probes
supernovae is and explosion of a massive giant star 41h 2he element mademass before helium red
supernovae is to compare a finding chart of a galaxy with a naked eye view at the telescope
supernovae is bluer than for the nearby sample could hint at evolutionary effects
supernovae is easy to see in the asiago supernova catalogue
supernovae is what synthesizes the production of the elements heavier than iron
supernovae is a vast
supernovae is a vast increase in brightness
supernovae is also a technical challenge
supernovae is usually the
supernovae is "a stupendous explosion of a massive
supernovae is a very rare form of iron
supernovae is simply the end of the life cycle of a star
supernovae is then expected to follow the differential volume curve
supernovae is also estimated
supernovae is important since
supernovae is neglected
supernovae is ejected
supernovae is calculated by co
supernovae is observed to be expanding at 5
supernovae is a plot of the intensity
supernovae is
supernovae is needed to produce cosmic rays
supernovae is revealed
supernovae is already on the way to us
supernovae is needed to address extinction
supernovae is detected by superkamiokande
supernovae is reexamined
supernovae is employed for the distant supernovae
supernovae is then recycled in stars
supernovae is polarized
supernovae is also relatively
supernovae is proposed
supernovae is measured using cepheid variables that reside in the same galaxy as the supernovae
supernovae is to find them
supernovae is more than any other living person and is surpassed only by the legendary fritz zwicky
supernovae is immediately to the lower left of the nucleus
supernovae is provided by mr
supernovae is emitted in an as
supernovae is limited by the sensitivity and resolution of current radio telescope arrays
supernovae is steep
supernovae is about equal
supernovae is added in
supernovae is visible
supernovae is quite small
supernovae is unresolved
supernovae is one of the primary science goals of ngst
supernovae is of the order of
supernovae is thus crucial to understanding how our part of the universe came to be
supernovae is that during the event they radiate as much energy in a very short time as the galaxy in which they reside
supernovae is derived in v and is
supernovae is stretched
supernovae is a binary system consisting of a orbiting a star
supernovae is recondensed into succeeding new stars and planets
supernovae is that the derived distances are independent of calibration from galactic measurements; the disadvantage is that the
supernovae is m~ 20 m
supernovae is therefore a direct measure of their relative
supernovae is where the hydrogen expires and the remaining helium turns into carbon and then eventually after a while into iron
supernovae is the rotation of the various layers of the star
supernovae is well known
supernovae is also being developed in new mexico
supernovae is the one of the most striking discoveries in cosmology
supernovae is a process of elimination
supernovae is called a light curve
Nickname supernovae
- supernovae (Points: 0)